Main physical properties used in our analysis. Panels above show spectroscopic redshift, stellar mass (log(M_star/M_⊙)), attenuation in the FUV band (A_FUV), SFR and specific SFR (sSFR), both in logarithmic scale. The last bottom right panel shows the axis ratio (semi-minor/semi-major) from Meert et al. (2015). Black histograms represent distributions obtained from the whole sample of 29 487 galaxies (0.01 < z < 0.30), while maroon hatched histograms show distributions for the final sample used for the analysis (7986 galaxies). Legends show median values for all parameters calculated for the initial (black histograms) and final (maroon hatched histograms) samples.