The galaxy presents as a fairly smooth, elliptical or lenticular system. It displays a notable central bulge that is bright and concentrated. There is little evidence of spiral arm structure or significant dust lanes, which further suggests a classification towards the elliptical end of the galaxy morphology spectrum. The color gradient transitions smoothly from a yellower core to redder outskirts, suggesting an older stellar population with less ongoing star formation. The galaxy does not appear to be significantly disturbed or undergoing a major merger event. The overall shape appears mostly round but is slightly elongated.
