  The photometric and morphological analysis of galaxies in clusters provides
invaluable information regarding the evolutionary stage of the cluster itself.
In addition, it helps to understand how the environment affects the properties
of the galaxies and, as a consequence, their evolutionary path. In this
contribution we present the first steps on the photometric and morphological
analysis of galaxies in the Fornax cluster using S-PLUS data. We expect that
the S-PLUS novel filter set and wide field coverage allow us to obtain new
information about Fornax and its galaxy population.
