  We investigate a simplified model for the strange stars in the framework of
Finslerian spacetime geometry, composed of charged fluid. It is considered that
the fluid consisting of three flavor quarks including a small amount of
non-interacting electrons to maintain the chemical equilibrium and assumed that
the fluid is compressible by nature. To obtain the simplified form of charged
strange star we considered constant flag curvature. Based on geometry, we have
developed the field equations within the localized charge distribution. We
considered that the strange quarks distributed within the stellar system are
compiled with the MIT bag model type of equation of state (EOS) and the charge
distribution within the system follows a power law. We represent the exterior
spacetime by the Finslerian Ressiner-Nordstr{\"o}m space-time. The maximum
anisotropic stress is obtained at the surface of the system. Whether the system
is in equilibrium or not, has been examined with respect to the
Tolman-Oppenheimer-Volkoff (TOV) equation, Herrera cracking concept, different
energy conditions and adiabatic index. We obtain that the total charge is of
the order of 10$^{20}$ C and the corresponding electric field is of around
10$^{22}$ V/m. The central density and central pressure vary inversely with the
charge. Varying the free parameter (charge constant) of the model, we find the
generalized mass-radius variation of strange stars and determine the maximum
limited mass with the corresponding radius. Furthermore, we also considered the
variation of mass and radius against central density respectively.
