This galaxy presents a generally smooth and elliptical morphology. It appears to be relatively undisturbed, showing no strong signs of ongoing or recent major merger activity. The galaxy exhibits a bright central bulge that dominates its luminosity profile, suggesting a significant concentration of older stars. The shape is more in between round and cigar shaped, with a slight elongation. The color profile indicates that the galaxy is redder, likely due to an older stellar population and lower levels of recent star formation. There is a very faint hint of a disk or faint feature around the center, but not by much.
