The galaxy appears as a relatively smooth, elliptical or lenticular structure. The light distribution is centrally concentrated, with a gradual decrease in surface brightness towards the outer regions. The color is generally consistent, showing a moderate level of star formation. There is no obvious spiral arm structure or significant dust lane features, but there is a slight asymmetry. There may be signs of a minor tidal disturbance, suggesting a possible past interaction with another galaxy, however the object is largely undisturbed and un-merged.
