The galaxy presents as a relatively smooth, elliptical or lenticular-like structure. Its overall color is a blend of yellow and white, suggesting a stellar population dominated by older stars and a low rate of ongoing star formation. The galaxy exhibits a concentrated central bulge, with a gradual decrease in luminosity towards its outer edges, indicating a lack of prominent spiral arms or distinct features. The round appearance suggests it lacks any significant disk-like structure. There is no indication of any major mergers, or any significant interaction occurring with neighboring galaxies or other external disturbances.
