The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge. It exhibits a yellowish hue, suggesting an older stellar population and reduced star formation. There is very little, if any, discernible disk structure. It appears relatively undisturbed, lacking any strong evidence of ongoing or recent major mergers. A minor asymmetry may be present in the outer regions, which could be indicative of past minor disturbances. The galaxy appears moderately rounded, not significantly elongated.
