  The present work contains a discussion on compact stellar body that is
influenced by the effects electromagnetic fields. We have tried to discuss a
solution of Einstein-Maxwell field equation with the interpretation of Buchdahl
spacetime type function. The interior fluid density and anisotropic pressures
have been derived for a charged fluid of compact body which is also continuous
with the Reissner-Nordstrom metric exterior solution. We have discussed the
singularity free interior anisotropic fluid under electromagnetic influence.
The thermodynamics energy conditions and their variation with interior radius
have been discussed here. We have also discussed the physical acceptability of
this new model. Finally we have included the scalar field theory corresponding
to the interior fluid that helped us to discuss teh compact body strange star
evolution with time. The generalized entropy evolution of the compact body has
also been introduced in the discussion of interior fluid evolution analysis
