The galaxy presents as a centrally concentrated elliptical morphology. It exhibits a smooth luminosity profile, lacking apparent spiral arm structures or significant dust lanes. The core region shows a bright, diffuse glow. The object appears subtly elongated. There is a noticeable color gradient, shifting from a yellower hue in the nucleus to a redder tone toward the outer edges. There is no sign of tidal disturbances or nearby galactic mergers. Overall, the object exhibits characteristics consistent with a mature, passively evolving system.
