The galaxy presents a generally smooth, rounded morphology. It exhibits a concentrated central bulge that appears yellowish in color, suggesting a population of older stars. There is a subtle color gradient from the center outwards, with the outer regions showing hints of bluer light, potentially indicative of some ongoing star formation, albeit at a low rate. There are no clearly discernible spiral arms or prominent dust lanes, but slight disturbances are visible. The object does not appear to be undergoing a major merger, though there may be minor interactions with smaller companions. The inferred size of the galaxy is roughly 6 kpc across, at a distance indicated by its redshift.
