The galaxy presents a predominantly smooth and rounded morphology, characteristic of an elliptical or lenticular galaxy. The central bulge exhibits a concentrated luminosity, suggesting a high stellar density. The overall color profile is indicative of an older stellar population, appearing more yellow and red than blue. There is little visible evidence of spiral arms or significant dust lanes, suggesting a lack of ongoing active star formation. There is a very slight potential that the galaxy is in the late stages of a minor merger, although the primary indication of this is a slight asymmetry of the disk that could simply be due to an uneven distribution of dust and gas.
