The galaxy appears to be a relatively smooth, elliptical-type galaxy. Its light profile is centrally concentrated, with a gradual decrease in brightness outwards, suggesting an older stellar population. There is some evidence of low level star formation activity present. The galaxy displays a nearly circular shape, which indicates it is close to spherical in its three-dimensional structure. There's no visible evidence of recent major merger events or significant tidal disturbances. It's color is slightly redder than the average galaxy, also suggesting that the galaxy has stopped forming stars.
