  The present work deals with a FLRW cosmological model with spatial curvature
and minimally coupled scalar field as the matter content. The curvature term
behaves as a perfect fluid with the equation of state parameter w_K = -1/3
Using suitable transformation of variables, the evolution equations are reduced
to an autonomous system for both power law and exponential form of the scalar
potential. The critical points are analyzed with center manifold theory and
stability has been discussed. Also, critical points at infinity have been
studied using the notion of Poincare sphere. Finally, the cosmological
implications of the critical points and cosmological bouncing scenarios are
discussed. It is found that the cosmological bounce takes place near the points
at infinity when the non-isolated critical points on the equator of the
Poincare sphere are saddle or saddle-node in nature.
