The galaxy presents an elliptical morphology, displaying a smooth and concentrated central bulge. The light distribution suggests a lack of significant spiral arm structures, instead showing a gradual decrease in luminosity from the core outwards. The galaxy appears to be slightly elongated. There may be minor disturbances occurring within the galaxy, but the core appears undisturbed. The overall color profile appears to be slightly redder in the central region, gradually becoming bluer toward the outer edges, perhaps indicative of a decrease in older stellar populations from the core.
