The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology is elliptical, showing a high degree of roundness. There is a slight color gradient, with a core region appearing more yellow, suggestive of an older stellar population, and the outer regions displaying a slightly bluer hue. No distinct spiral arms, bar structures, or prominent dust lanes are visible. The galaxy does not appear to be strongly interacting or undergoing a major merger, although there are some subtle indications of minor disturbances in its overall structure. The galaxy appears to be relatively compact, having a moderate size.
