  In this paper, we have presented a bouncing cosmological model of the
Universe in an extended theory of gravity. The dynamical behaviour of the model
obtained from the flat FLRW space-time along with the violation of null energy
condition have been shown. The geometrical parameters show singularity
behaviour at the bouncing epoch. The parameters involved in the scale factor
play a major role in the bouncing behaviour. In addition, the coupling
parameter that resulted in the minimal matter-geometry coupling in the extended
gravity has significant role to avoid the singularity of equation of state
parameter at the bouncing epoch. Using a linear homogeneous perturbation
calculation, we show the stability of the model.
