  The role played by the large-scale structures in the galaxy evolution is not
quite well understood yet. In this study, we investigate properties of galaxy
in the range 0.1<z<0.3 from a value-added version of the WISExSCOS catalogue
around cosmic filaments detected with DisPerSE. We have fitted a profile of
galaxy over-density around cosmic filaments and found a typical radius of r_m =
7.5+-0.2 Mpc. We have measured an excess of passive galaxies near the
filament's spine, higher than the excess of transitioning and active galaxies.
We have also detected SFR and Mstar gradients pointing towards the filament's
spine. We have investigated this result and found an Mstar gradient for each
type of galaxies: active, transitioning, and passive, and a positive SFR
gradient for passive galaxies. We also link the galaxy properties and the gas
content in the Cosmic Web. To do so, we have investigated the quiescent
fraction fQ profile of galaxies around the cosmic filaments. Based on recent
studies about the effect of the gas and of the Cosmic Web on galaxy properties,
we have modeled fQ with a beta model of gas pressure. The slope obtained here,
beta=0.54+-0.18, is compatible with the scenario of projected isothermal gas in
hydrostatic equilibrium (beta=2/3), and with the profiles of gas fitted in SZ.
