Metformin is widely recognized as a primary medication in the global management of type 2 diabetes mellitus (T2DM), earning its inclusion on the World Health Organization’s list of essential medicines since 2019 [
1]. Its low cost, excellent tolerability, and safety profile, with low risk of hypoglycemia, make it a preferred choice either alone or in combination with other drugs for managing millions of patients with T2DM [
2]. Metformin belongs to the biguanide family (1,1-dimethylbiguanida hydrochloride) originating from the plant known as French lilac (
Galega officinalis) [
3]. Historically, this plant has been utilized in Europe since the Middle Ages to alleviate symptoms of diabetes mellitus, owing to its abundance of galegine, an isoprenyl guanidine compound. While monoguanidines and diguanidines exhibit toxicity, biguanides, composed of two N-linked guanidine molecules, have been employed for diabetes treatment since the late 1950s [
4]. Metformin gained approval for use in Europe and Canada in 1957, not being introduced in the United States until 1995 [
3]. The more potent biguanides, phenformin and buformin, were widely used in the United States and Europe in the 1960s, however, they were withdrawn from the market in the late 1970s due to a higher risk of lactic acidosis compared to metformin (approximately 3-9 cases per 100,000 person-years). Notably, the risk of lactic acidosis is elevated in patients with chronically impaired renal function or acute kidney disease, populations for whom metformin is contraindicated [
5]. Consequently, the most prevalent adverse effect associated with metformin is gastrointestinal intolerance [
6].
Although metformin has been administered to millions of patients with T2DM for over 60 years, the exact mechanism (or mechanisms) of action remains a subject of debate. Metformin is described as an anti-hyperglycemic agent that does not induce clinical hypoglycemia in patients with T2DM or disturb glucose homeostasis in non-diabetic individuals [
2,
7]. It is known that metformin primarily acts by suppressing hepatic glucose production, which is increased in individuals with T2DM, through a decrease of 25-40% in the hepatic gluconeogenesis rate [
8]. Additionally, some euglycemic-hyperinsulinemic clamp studies suggest it may also have a beneficial effect on insulin sensitivity at the skeletal muscle level, although this effect is not consistently observed across all studies [
9,
10,
11,
12]. In recent years, a growing body of evidence points to the gut as a key target of metformin action, promoting glucose utilization, GDF15 secretion, which reduces appetite, and regulating intestinal microbiota, all of which collectively contribute to its potential benefits (reviewed in (Barroso et al., 2023) [
13]).
Controversy surrounds the primary targets of metformin to promote the reduction in hepatic gluconeogenesis. For over 50 years, it has been known that biguanides decrease mitochondrial respiration, thus placing mitochondria at the core of their action [
14]. However, the precise molecular targets within this organelle and their subsequent effects are diverse, leading to a plethora of proposed mechanisms, some of which may overlap, in explaining metformin’s antigluconeogenic effects in the liver. Notably, inhibition of mitochondrial respiratory chain Complex I and mitochondrial glycerophosphate dehydrogenase are prominent among these targets, although other respiratory chain complexes have also been suggested as potential targets [
15,
16,
17]. Metformin’s impact on these targets manifests in a complex array of interconnected effects, including cellular energy deficits, changes in the redox state, activation of AMP-activated protein kinase (AMPK), inhibition of cAMP-mediated glucagon signaling, allosteric modulation of gluconeogenic enzymes, as well as epigenetic alterations [
18,
19]. Untangling which of these events truly drives the reduction in hepatic gluconeogenesis induced by metformin remains a subject of intense debate. Moreover, the fact that many of metformin’s effects seen in in vitro and preclinical studies occur at suprapharmacological concentrations, coupled with discrepancies in effects between acute and chronic administration in in vivo models, further complicates the interpretation of these findings and, consequently, the elucidation of the underlying molecular mechanisms of this drug. Investigation into the underlying molecular mechanisms of action of metformin has garnered significant interest beyond its applications in diabetes treatment. Metformin’s capacity to alter cellular bioenergetics and modulate crucial aspects of mitochondrial function, such as oxidative stress and apoptosis, has sparked curiosity about its potential repurposing in treating various diseases [
18]. Notably, there is growing enthusiasm for exploring metformin’s potential as a therapeutic agent against certain types of cancer, such as breast and colon cancer [
20,
21,
22]. One of the hallmarks of cancer is the reprogramming of cellular energy metabolism, allowing tumor cells to sustain continuous growth and proliferation by substituting the metabolic program typically found in normal tissues. Drugs like metformin, with the ability to exploit specific metabolic vulnerabilities in tumor cells, present a promising avenue for cancer treatment [
23]. Indeed, lower incidences of certain types of cancer and/or improved overall survival has been reported in T2DM patients treated with metformin [
22,
24,
25]. Repurposing existing drugs for other diseases offers significant time and cost-saving advantages, as their pharmacokinetics, pharmacodynamics, and safety profiles are already established, thus allowing preclinical studies to be streamlined. Given the considerable interest in metformin, this review aims to delve into the current understanding of its mechanisms of action and its potential applications in breast and colon cancer treatment. Furthermore, we will examine the primary challenges associated with repurposing metformin for cancer therapy and discuss the strategies being contemplated to address these challenges.
1.1. Pharmacokinetics
Metformin is characterized chemically as a highly hydrophilic compound with an acid dissociation constant (pKa) of 11.5, meaning that at physiological pH the drug exists as a monoprotonated cation. The presence of charge at physiological pH results in two main consequences: drug transport across biological membranes involves uptake via specific transporters, and organelles such as energized mitochondria, can slowly accumulate the drug driven by their transmembrane electrochemical potential (Δψ) [
26]. Thus, it is known that the absorption, distribution, and excretion of metformin primarily rely on organic cation transporters (OCTs), multidrug and toxin extruders (MATEs), and plasma membrane monoamine transporter (PMAT) [
27,
28].
Metformin is typically administered orally and exhibits a low bioavailability ranging from 40% to 60% [
29]. The drug is not metabolized and is excreted unchanged through urine. In the treatment of T2DM, patients are typically prescribed a dosage of 25-30 mg/kg per day, typically divided into two or three oral doses of 500-850 mg each. However, it’s important to note that the absorption of metformin is reliant on specific transporters and, therefore, administering higher doses can slow the absorption rate and decrease overall bioavailability [
30]. In mouse models, higher doses (200-250 mg/kg) are often necessary due to their more efficient renal clearance, resulting in a shorter half-life of 1-2 hours compared to the 4-9 hours observed in humans [
31]. Biodistribution studies in humans, employing positron emission tomography (PET) with
11C-labeled metformin, demonstrate its primary distribution in the small intestine, liver, and kidneys. This distribution pattern aligns with both the expression profile of previously discussed specific transporters and the major target organs (liver and gut), as well as its high rate of renal elimination [
27,
32]. Following intestinal absorption, metformin attains high concentrations in the portal vein (40-70 µM), leading to the accumulation of higher levels of metformin in the liver than in surrounding organs, as confirmed by PET in in both humans and mice [
17,
33,
34]. It is noteworthy that studies in mice indicate that the liver can reach concentrations even higher than those in portal vein plasma [
35].
In this sense, it is important to emphasize that antineoplastic effects of metformin depend on drug concentration within neoplastic tissue. This concentration is influenced not only by plasma level, but also by cellular uptake in cancer cells, which depends on the expression of relevant transporters including OCT1 [
36]. It is worth noting that serum levels of metformin achieved in diabetic patients and in vivo models are in the micromolar range, while in vitro antitumoral activity is observed at millimolar concentrations [
37]. Hence, a fundamental research inquiry is to determine the metformin concentrations achieved in tumors of patients receiving conventional antidiabetic metformin dose.