The galaxy presents as a fairly compact, elliptical system. It exhibits a centrally concentrated luminosity profile, with a smooth, diffuse appearance suggesting a lack of significant spiral arm structure or prominent dust lanes. The core region appears bright and slightly bluish, potentially indicative of ongoing star formation, though the overall colour suggests an older stellar population dominating the galaxy. The galaxy appears fairly isolated, with no obvious signs of tidal interactions or ongoing mergers. The overall morphology is well-rounded, with no apparent elongation.
