The galaxy appears as a centrally concentrated object, approximately elliptical in shape. It exhibits a smooth, diffuse light distribution, with a bright core that gradually fades outwards. No distinct spiral arms or prominent dust lanes are discernible in the image. There is a hint of a slightly more extended, diffuse halo surrounding the central region. Overall, it seems relatively undisturbed, showing no major signs of ongoing mergers or tidal interactions, but possibly some minor disturbances. The galaxy's colour profile is indicative of a mature stellar population, potentially composed of older, redder stars, with low levels of active star formation.
