The galaxy presents as a moderately luminous object with a discernible, centrally concentrated bulge. The galaxy has an elliptical morphology, exhibiting a smooth profile without prominent spiral arms or a distinct disk structure. The central region displays a yellowish-white hue, suggestive of an older stellar population. The outer regions appear fainter with a slightly bluer tint, possibly indicating the presence of younger stars or ongoing star formation, though the overall star formation activity appears to be relatively low. There is some evidence of minor disturbance of the galaxy, such as tidal tails, suggesting it may have undergone a recent interaction. The overall shape of the galaxy is not perfectly round, but exhibits a slight elongation, indicating a shape that falls between round and cigar-shaped.
