The galaxy exhibits a morphology tending towards smooth, with a central bulge that appears to be a dominant feature. The overall color profile suggests a galaxy with a significant population of older stars, particularly concentrated in the bulge, as indicated by the yellowish hue. The outer regions show a bluer tint, hinting at the presence of younger stellar populations and possibly ongoing star formation, although the rate appears to be relatively moderate. There is some suggestion of a disk structure, but this is not distinctly pronounced. There are no immediately apparent signs of major mergers or significant tidal disturbances, but a minor disturbance cannot be ruled out based on this imagery alone. The object's apparent symmetry and lack of strong irregularities suggest a galaxy that is relatively settled in its evolution.
