This galaxy appears to be a relatively smooth, elliptical type galaxy. It exhibits a concentrated central bulge with a gradual decrease in surface brightness towards its outer regions. The galaxy presents a predominantly yellow-orange hue, suggesting an older stellar population with a relatively low rate of ongoing star formation. There's no discernible spiral arm structure or dust lanes visible. The morphology is generally rounded, showing no significant signs of tidal disruption or interaction with other galaxies, although there are some possible disturbances visible. The overall impression is that of a passively evolving, massive galaxy.
