The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge that is bright yellowish-orange, suggesting an older stellar population with relatively low star formation activity. The galaxy is fairly symmetrical and round. There are no indications of any significant tidal disturbances, merging events, or spiral arm structures. The outer regions appear fainter and somewhat bluer, indicative of a small amount of recent star formation or a population of slightly younger stars in the galactic halo. Overall, the galaxy appears to be a fairly evolved system.
