  The observed properties of galaxies are strongly dependent on both their
total stellar mass and their morphology. Furthermore, the environment is known
to play a strong role in shaping them. The galaxy population in the local
universe that is located in virialized clusters is found to be red, poorly
star-forming, and mostly composed of early morphological types. Towards a
holistic understanding of the mechanisms that drive galaxy evolution, we
exploit the spectrophotometric data from the WINGS and OmegaWINGS local galaxy
cluster surveys, and study the role of both the local and the large-scale
environments. We attempt to disentangle their effects from the intrinsic
characteristics of the galaxies, in shaping the star formation activity at
fixed morphological type and stellar mass. Using a sample of field galaxies
from the same surveys for comparison, we analyse the effects of the
environment, embodied by the local density, clustercentric distance, and close
neighbours, respectively, on the star formation histories of cluster galaxies.
We find that local effects have a more relevant impact on galaxy stellar
properties than the large-scale environment, and that morphology needs to be
taken into account to pinpoint the mechanisms that are driving the influence of
clusters in galaxy evolution.
