The galaxy presents as a relatively smooth, centrally concentrated object. Its light profile suggests a dominant spheroidal component. The galaxy exhibits a yellowish-white hue, potentially indicating an older stellar population with fewer young, massive stars contributing to the overall color. There is a slight elongation to the shape, but it appears mostly rounded. Faint disturbances or tidal features are not readily apparent in the image, implying it is not undergoing a major merger or significant interaction with another galaxy. Star formation is not evident in the image.
