The galaxy exhibits a generally smooth morphology. The light profile suggests an elliptical or lenticular type. There is a bright, concentrated core region that gradually diffuses outward. The galaxy appears relatively round, with no obvious signs of strong tidal interactions or major disturbances. Its color suggests it consists primarily of older stellar populations, showing a reddish-orange hue in its central regions transitioning into a dimmer, slightly greener periphery. Any spiral arm structures or dust lanes are either absent or unresolved at this resolution.
