  In this work, we have studied how incorporating viscous fluids leads to exact
bounce cosmological solutions in general relativity (GR) framework.
Specifically, we propose a novel parameterization of bulk viscosity coefficient
of the form $\zeta = \zeta_0 (t-t_0)^{-2n} H$, where $\zeta_0$, $n$ being some
positive constants and $t_0$ is the bounce epoch. We investigate how this form
of bulk viscosity may assist in explaining the early universe's behaviour, with
a particular focus on non-singular bounce scenario by studying the various
energy conditions and other related cosmological observables and how the model
parameters affect the evolution of the Universe. We demonstrate that the NEC
and SEC violation occurs at the bounce point while DEC is satisfied. Finally,
we carried out a stability check based on linear order perturbation to the
Hubble parameter. We found that the perturbation vanishes asymptotically at
later times, which indicates a stable behaviour of the bounce scenario
