The galaxy presents as a primarily smooth, elliptical structure. There is a slight flattening of the galaxy, suggesting it is not a perfect sphere, but it lacks any discernible spiral arm structures. The core region appears bright and somewhat compact with a bright red area, potentially indicative of a high concentration of older stars or significant dust obscuration. Moving outward from the core, the galaxy exhibits a diffuse, greenish halo. The smooth light distribution of the greenish halo suggests an older stellar population. There is evidence of minor disturbances in the outer regions of the galaxy. The overall color profile of the galaxy suggests a stellar population consisting of a mix of old and new stars, and a non-negligible amount of dust.
