The galaxy presents a largely elliptical morphology. It appears relatively smooth in structure, with a highly concentrated central bulge. There is a clear color gradient, with the core exhibiting a yellowish hue, which suggests a population of older stars dominating the central region. Proceeding outwards from the core, the color shifts towards a more greenish tone. This could indicate the presence of a younger stellar population in the outer regions, or possibly some ongoing, albeit low-level, star formation. There are no visible dust lanes or spiral arm structures. The overall appearance is consistent with an early-type galaxy.
