The galaxy presents as a relatively smooth, elliptical-like system. It exhibits a centrally concentrated luminosity profile, appearing brightest towards the core and gradually fading outwards. The color gradient suggests a somewhat redder core region, possibly indicating an older stellar population or increased dust extinction in the center. Some bluer features are observed in the outer regions, hinting at the presence of younger stars or ongoing star formation there, although the overall star formation rate is relatively low. There is a slight asymmetry or minor disturbance in the overall structure, but the galaxy does not appear to be undergoing a major merger or strong tidal interaction. The isophotes are generally elliptical in shape, though deviations indicate that the galaxy is not perfectly spheroidal or disk-like.
