  We study a cosmological setup consisting of a FRW metric as the background
geometry with a massless scalar field in the framework of classical
polymerization of a given dynamical system. To do this, we first introduce the
polymeric representation of the quantum operators. We then extend the
corresponding process to reach a transformation which maps any classical
variable to its polymeric counterpart. It is shown that such a formalism has
also an analogue in terms of the symplectic structure, i.e., instead of
applying polymerization to the classical Hamiltonian to arrive its polymeric
form, one can use a new set of variables in terms of which Hamiltonian retains
its form but now the corresponding symplectic structure gets a new deformed
functional form. We show that these two methods are equivalent and by applying
of them to the scalar field FRW cosmology see that the resulting scale factor
exhibits a bouncing behavior from a contraction phase to an expanding era.
Since the replacing of the big bang singularity by a bouncing behavior is one
of the most important predictions of the quantum cosmological theories, we may
claim that our polymerized classical model brings with itself some signals from
quantum theory.
