The galaxy presents a generally smooth appearance with a concentrated central bulge. There is evidence of a surrounding disk component, though it appears faint and relatively undisturbed. The galaxy exhibits a moderately elliptical shape, appearing neither perfectly spherical nor highly elongated. The light profile suggests a higher concentration of older stars in the central region, with potentially some ongoing star formation in the outer disk, indicated by subtle variations in color. No major tidal features or signs of ongoing mergers are readily apparent. Faint color variations hint at differing stellar populations throughout the galaxy.
