The galaxy presents as a moderately luminous, elliptical-shaped system. Its core exhibits a bright, concentrated intensity, suggesting a high density of stars in the central region. The luminosity gradually decreases from the core outwards, forming a diffuse halo. Color gradients are subtle, with the central region appearing slightly more yellow, potentially indicating an older stellar population. The outer regions exhibit a bluer hue, but overall, the galaxy has a relatively smooth appearance, with no clear spiral arm structures or distinct dust lanes visible. There is a subtle suggestion of a disk, but no definitive spiral pattern. Minor disturbances in the form of light irregularities are present, which could suggest past minor interactions with other systems.
