The galaxy presents as a single, relatively smooth, centrally concentrated object with an elliptical morphology. It exhibits a dominant yellowish-orange hue, indicative of an older stellar population. There are two distinct brighter areas within the main body, potentially representing galactic nuclei undergoing a merger event. The overall light distribution is fairly symmetrical, with no apparent spiral arms or significant dust lanes visible. Faint, diffuse extensions seem to emerge, hinting at tidal interactions or ongoing mergers. No pronounced star forming regions are apparent.
