The galaxy appears to be a relatively smooth, elliptical type galaxy. It exhibits a centrally concentrated light profile with a gradual decrease in luminosity towards its outer regions. The overall shape is somewhat elongated, but more ovoid than cigar-shaped. There is no discernible spiral structure or prominent disk. The color is slightly redder, indicating an older stellar population and potentially lower ongoing star formation activity. There are no obvious signs of recent major merger activity or significant tidal disturbances, although a very subtle, minor perturbation cannot be ruled out. Overall, the galaxy presents as a fairly quiescent system.
