Note: Please see manuscript pdf for full abstract with equations. we introduce a new class of interior solutions that are singularity free and useful for describing genuine anisotropic compact starobjects with spherically symmetric matter distribution. we have considered metric potential selecting B2(r)=1/(1-r2/R2)n,where n >2. The various physical characteristics of the model were specifically examined for the pulsar PSRJ1903 + 327 with its currentestimated data. According to analysis, every physical need for aphysically admissible star is satisfied and all features are acceptable.Further the stability of the model is examined. Numerous pertinent physical characteristics are also highlighted in graphical form.