  In this paper, in an extended theory of gravity, we have presented bouncing
cosmological model at the backdrop of an isotropic, homogeneous space-time, in
presence of general relativistic hydrodynamics (GRH). The scale factor has been
chosen in such a manner that with appropriate normalization, the quintom
bouncing scenario can be assessed. Accordingly, the bounce occurs at $t=0$ and
the corresponding Hubble parameter vanishes at the bounce epoch. The equation
of state (EoS) parameter and the energy conditions of the model have been
analysed. The violation of strong energy condition further supports the
behaviour of extended gravity. As the bouncing cosmology suffers with
instability, this model also shows the similar behaviour.
