This galaxy presents as a relatively smooth, lenticular-like structure with an apparent intermediate axis ratio. The light distribution is centrally concentrated, with a gradual falloff in surface brightness towards the outer regions. The core region appears yellowish-white and slightly more luminous than the outer regions. There is a subtle bluer color visible on the outskirts of the galaxy, possibly indicating a small amount of ongoing star formation. The overall morphology suggests a relatively evolved system, with the bulk of star formation having ceased. There is a hint of possible distortion, indicating a past interaction or merger event. However, there are no tidal tails or other clear signs of strong gravitational disturbance.
