The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a bright, concentrated luminosity, suggestive of a dense stellar population or active galactic nucleus. Moving outwards from the core, the light gradually diminishes, transitioning into a more diffuse halo. There are faint indications of a slightly elongated shape, but overall the object appears largely spheroidal. No spiral arms or distinct features are readily discernible. The galaxy shows a subtle color gradient, with the core appearing slightly yellower, potentially indicating an older stellar population, while the outer regions appear bluer. No signs of any major mergers or tidal disturbances are apparent.
