The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central region, suggesting a significant bulge component. The color is generally blue-white, potentially indicating the presence of a younger stellar population, even if it's an elliptical galaxy. There is a lack of defined spiral arms or prominent dust lanes, reinforcing the classification of a smooth galaxy. The galaxy appears relatively isolated, showing no clear signs of ongoing major merger activity, although there might be very faint disturbances. Its overall structure suggests a system that has largely completed its major evolutionary processes.