The galaxy presents a generally smooth morphology, with a dominant central bulge that appears relatively round. There is a slight suggestion of a disk component, although it is not prominent. The color profile indicates a population of older stars, particularly concentrated in the central region, as indicated by the reddish-yellow hue. There's a subtle bluer component, possibly indicating recent or ongoing star formation. It appears relatively undisturbed, with no major signs of ongoing merging activity or tidal disruption. 
