This galaxy exhibits a generally smooth morphology, indicative of an elliptical galaxy. It displays a high degree of circularity, appearing nearly round in shape. There is no discernible disk structure or spiral arms. The galaxy appears relatively undisturbed, showing no significant signs of ongoing or recent major mergers, although a faint hint of minor disturbance cannot be entirely ruled out. Color gradients suggest a relatively uniform stellar population. A high apparent brightness suggests a relatively close distance.
