The galaxy appears to be a relatively smooth, elliptical galaxy, possibly of type E0-E3. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards the outer regions. There is no apparent disk structure, spiral arms, or dust lanes visible. The galaxy displays a yellowish-orange hue, suggesting an older stellar population with a low rate of ongoing star formation. There is no significant evidence of tidal tails or other distortions indicative of recent mergers or interactions, though there are a few faint areas on the edge that could suggest minor disturbances. The galaxy has a fairly high degree of roundness. 
