The galaxy presents an elliptical morphology, with a predominantly smooth light distribution across its body. The color profile suggests an older stellar population, appearing more reddish-yellow in the central region. There is no distinct disk structure visible. A fainter, bluish component is located in close proximity, and the overall impression is that the galaxy is interacting, or has interacted in the past, with another galactic object. This could suggest a potential minor merger event, although no tidal tails or other strong distortions are clearly visible. It is a massive galaxy with very low star formation, composed of older stars.
