Distributions of stellar mass (left column), (g − r)₀ colour (middle column), and bulge prominence (right column) for AGNs (top row), star-forming galaxies (middle row), and undetermined galaxies (bottom row). We show strongly barred galaxies in solid red lines, weakly barred in dashed navy blue, and unbarred in dotted teal. The AGNs tend to have higher bulge prominences, redder colours, and higher stellar masses than their star-forming counterparts, although the ranges of these parameters do not vary significantly. The differences between the bar strengths are more apparent in star-forming galaxies than in AGNs, with bulge prominence being particularly divided in undetermined galaxies.