The galaxy presents a moderately inclined, elongated morphology, suggesting a potential classification as an elliptical galaxy. The light profile shows a concentration towards the center, with a smooth, diffuse halo extending outwards. The central region appears relatively bright, but not indicative of an Active Galactic Nucleus.

There are subtle hints of substructure within the galactic disk, possibly representing regions of enhanced star formation or dust lanes, but these features are not sharply defined. No prominent spiral arms or bar structures are observed. The overall color appears moderately red, suggesting a population of older stars and/or significant dust obscuration. There is a possible merging event occurring, or possibly some tidal distortion.
