  We studied a new class of interior solutions that are singular-free and
useful for describing anisotropic compact star objects with spherically
symmetric matter distribution. We have considered metric potential selecting
B_0^2 (r)=1/(1-r^2/R^2 )^n ,where n>2 . The various physical characteristics of
the model are specifically examined for the pulsar PSRJ1903+327 with its
current estimated data. According to analysis, every physical need for a
physically admissible star is satisfied and all features are acceptable.
Further, the stability of the model has been examined. Numerous physical
characteristics are also highlighted in a graphical form.
