Global stellar population properties as a function of the Hubble type obtained with a delayed-τ model and Chabrier IMF. From top to bottom we show the galaxy stellar mass (M_⋆), attenuation (τ_V), light-weighted averaged age (), and stellar metallicity (⟨log Z⟩). The individual galaxy values are plotted as gray dots, and the average values for each Hubble type are shown as color-coded stars.