  Galaxy clusters are the largest gravitationally bound systems in the Universe
and, as such, play an important role in cosmological studies. An important
resource for studying their properties in a statistical manner are homogeneous
and large image datasets covering diverse environments. In this sense, the
wide-field images (1.4 deg^{2}) obtained by the Southern Photometric Local
Universe Survey (S-PLUS) in 12 optical bands, constitute a valuable tool for
that type of studies. In this work, we present a photometric analysis of pixel
color-magnitude diagrams, corresponding to a sample of 24 galaxies of different
morphological types located in the Fornax cluster.
