The galaxy presents as a largely smooth, elliptical-like structure. Its core exhibits a bright, concentrated luminosity, indicating a high density of stars in the central region. The galaxy gradually fades in intensity from the center outwards, lacking any distinct spiral arm structures or prominent dust lanes. The overall color profile suggests a population of older stars, with a yellowish-red hue dominating. There are some indications of slightly bluer regions in the outskirts of the galaxy which indicates pockets of ongoing or recent star formation but they are very diffuse. The morphology suggests a relaxed system, without significant signs of recent mergers or major disturbances. The overall roundness of the galaxy is apparent, with a minor deviation from a perfect circular shape. No evidence of a bar structure is discernible.
