This study explores the characteristics of anisotropic spherically symmetric stellar structures in the context of modified $f(R, T)$ gravity, a theory that aims to address some of the enduring experimental difficulties, such as the universe's dark region. The authors investigate how the fluid distribution in the star model is affected by the MIT bag model equation of state to explain the unique properties of compact objects. Using Tolman V metric potentials, they establish the field equations and identify the values of unknown parameters by employing experimental data from observed stars. They further examine the effects of energy density, anisotropic factor, transversal and radial pressure within the cores of these stars for a specific Bag constant. The stability of the cosmic structure and the physical validity of the model are assessed through equilibrium conditions, energy, and causality parameters. The study concludes that the physical conditions are satisfied by the model, and the magnitude of the Bag constant agrees with experimental data, demonstrating the model's feasibility.This study explores the characteristics of anisotropic spherically symmetric stellar structures in the context of modified $f(R, T)$ gravity, a theory that aims to address some of the enduring experimental difficulties, such as the universe's dark region. The authors investigate how the fluid distribution in the star model is affected by the MIT bag model equation of state to explain the unique properties of compact objects. Using Tolman V metric potentials, they establish the field equations and identify the values of unknown parameters by employing experimental data from observed stars. They further examine the effects of energy density, anisotropic factor, transversal and radial pressure within the cores of these stars for a specific Bag constant. The stability of the cosmic structure and the physical validity of the model are assessed through equilibrium conditions, energy, and causality parameters. The study concludes that the physical conditions are satisfied by the model, and the magnitude of the Bag constant agrees with experimental data, demonstrating the model's feasibility.