The galaxy presents as a slightly elongated, elliptical form. It exhibits a smooth light profile, suggesting a lack of significant spiral arm structures or prominent dust lanes. The core region appears significantly brighter and more concentrated than the outer regions, indicative of a central bulge. The overall color is yellowish-orange, implying a stellar population dominated by older, redder stars. There are subtle irregularities in the outer regions that suggest a possible recent or ongoing merger event or tidal interactions with another galaxy. There is a slight hint of disc structure when the image is zoomed.
