The galaxy presents a smooth, elliptical morphology. It exhibits a concentrated central bulge that dominates its overall structure. The light is distributed relatively evenly across the visible body of the galaxy, with a gradual decrease in intensity from the core to the outer edges. There is no evidence of spiral arms or a distinct disk component. The galaxy appears to be fairly round, with only a slight deviation from perfect circularity. No signs of ongoing mergers or major tidal disturbances are apparent. The dominant color is yellowish-orange, possibly indicating an older stellar population and relatively low star formation activity. There may be some subtle color variations in the outer regions, indicating some spatial distribution of stellar populations.
