The galaxy presents as an elliptical structure. The light distribution is centrally concentrated, with a smooth gradient outwards, indicating an evolved stellar population. The morphology is not perfectly elliptical; the isophotes appear somewhat disturbed, possibly due to tidal interactions or a recent minor merger. There is a slight asymmetry in the outer regions, with a faint extension or plume visible. The colour appears relatively uniform across the galaxy, with a redder hue. This indicates a relatively quiescent galaxy with ongoing but low levels of star formation.
