  This work is a Brazilian-Indian collaboration. It aims at investigating the
structuralproperties of Lenticular galaxies in the Stripe 82 using a
combination of S-PLUS (Southern Photometric Local Universe Survey) and SDSS
data. S-PLUS is a noveloptical multi-wavelength survey which will cover nearly
8000 square degrees of the Southern hemisphere in the next years and the first
data release covers the Stripe 82 area. The morphological classification and
study of the galaxies' stellar population will be performed combining the
Bayesian Spectral type (from BPZ) and Morfometryka (MFMTK) parameters. BPZ and
MFMTK are two complementary techniques, since the first one determines the most
likely stellar population of a galaxy, in order to obtain its photometric
redshift (phot-z), and the second one recovers non-parametric morphological
quantities, such as asymmetries and concentration. The combination ofthe two
methods allows us to explore the correlation between galaxies shapes (smooth,
with spiral arms, etc.) and their stellar contents (old or young population).
The preliminary results, presented in this work, show how this new data set
opens a new window on our understanding of the nearby universe.
