Location of galaxies from the H sample with varying mass-weighted B/T on the UVJ diagram (left: B/T< 0.2, middle: 0.2 <B/T< 0.6, right: B/T> 0.6), using the total magnitudes of each galaxy. The dotted line shows the dividing line between the star-forming and quiescent populations defined in Eq. (1). It is clear that both bulge- and disk-dominated galaxies occupy very different regions of the diagram, illustrating the good agreement between the colors and morphology. Intermediate galaxies with roughly equal mass in the disk and bulge (middle panel, ⟨B/T⟩ = 0.4) are spread over the two regions, with a tendency for being preferentially in the quiescent region.