The galaxy presents an elliptical morphology, exhibiting a smooth and somewhat diffuse appearance. The central region displays a high concentration of luminosity, suggesting a substantial stellar population and potentially a supermassive black hole at its core. The overall color index indicates a relatively evolved stellar population, trending towards redder hues, typical of older stars. There is a slight asymmetry in the outer isophotes, which could suggest either tidal interactions or an internal disturbance but the galaxy generally appears relaxed. There is a notable absence of prominent spiral arms or significant dust lanes, further supporting classification as an elliptical. The galaxy is moderately sized, with a significant fraction of the light coming from the central region, hinting at a lack of ongoing, significant star formation within the visible structure.
