The galaxy presents a largely smooth, elliptical morphology. The core exhibits a bright, concentrated luminosity, suggesting a relatively high stellar density or possible AGN activity, though not immediately apparent. The light profile decreases gradually from the core outward, exhibiting a fuzzy or diffuse halo region. There is a subtle color gradient visible, with the central region displaying a slightly yellower or redder hue, potentially indicating an older stellar population or dust obscuration. The outer regions appear bluer, possibly representing younger stars; this is subtle. No strong tidal features or evidence of recent mergers are readily apparent.
