The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It exhibits a yellowish-orange hue, suggesting an older stellar population with a lower rate of ongoing star formation. The galaxy's shape is mostly round, with only a slight deviation from perfect circularity. No distinct spiral arms or bar structures are visible. There is no evidence of significant tidal disturbances or mergers in progress; the galaxy appears relatively undisturbed and relaxed. The brightness profile suggests a smooth transition from the bright central core to the fainter outer regions.
