The galaxy appears to be a relatively smooth, elliptical-like object. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. The galaxy presents an overall yellow-white hue, suggesting an older stellar population with fewer ongoing star-forming regions. There is no distinct disk structure or spiral arm features visible. The galaxy appears to be fairly symmetrical. There are no obvious signs of recent major mergers or significant tidal disturbances.
