The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that gradually diffuses outward. The color is predominantly yellow-orange, indicating an older stellar population with lower rates of star formation. There is little evidence of spiral arms or dust lanes. The galaxy appears relatively isolated, showing no obvious signs of tidal interactions or major disturbances, though a very minor asymmetry could be present. It presents an overall rounded shape, with only a slight deviation toward an elongated form.
