The galaxy presents as a relatively smooth, elliptical-like structure. There is a central, concentrated bulge that appears yellowish, suggesting a population of older stars. The outer regions exhibit a bluer hue compared to the core, which could indicate the presence of some younger stars. The morphology suggests this galaxy is likely a relatively undisturbed system, not currently undergoing any major merging events, though there is the possibility of a minor interaction. The galaxy's overall form appears somewhat rounded, exhibiting a slight elongation.
