  We provide a new class of interior solution of a (2 + 1) dimensional
anisotropic star in Finch and Skea spacetime corresponding to the BTZ black
hole. We have developed the model by considering the MIT bag model EOS and a
particular ansatz for the metric function $ g_{rr}$ proposed by Finch and Skea
\cite{FS}. Our model is free from central singularity and satisfied all the
physical requirements for the acceptability of the model.
