The galaxy appears as a relatively compact, luminous object. Its overall morphology is smooth and elliptical in nature, lacking any discernible spiral arm structures or a prominent central bulge. The light distribution suggests a moderately concentrated core region that gradually fades towards the outer edges. The shape appears to be somewhere between perfectly round and more elongated, with the major axis only slightly longer than the minor axis. There is some subtle asymmetry in the outer isophotes, but these are not indicative of a major ongoing merger event. Instead, this likely indicates a minor interaction or internal disturbance of the galaxy. The overall color seems to indicate that the galaxy consists mainly of older stars with only a few areas of active star formation.
