The galaxy presents as a singular, relatively symmetrical object. The morphology appears largely smooth and rounded. There is a lack of discernible spiral arm structure or significant irregularities in its form. The central region exhibits a concentration of luminosity, suggesting a possible bulge. There are no apparent tidal tails or other major disturbances indicative of recent or ongoing mergers, though some minor disturbances cannot be ruled out. The color profile suggests a population of older stars, with a relatively low rate of on-going star formation. The galaxy displays an elliptical or lenticular profile, with an estimated size of approximately 4.5 kpc.
