  Collapsing process is studied in special type of inhomogeneous spherically
symmetric space-time model (known as IFRW model), having no time-like Killing
vector field. The matter field for collapse dynamics is considered to be
perfect fluid with anisotropic pressure. The main issue of the present
investigation is to examine whether the end state of the collapse to be a naked
singularity or a black hole. Finally, null geodesics is studied near the
singularity.
