The galaxy appears to be a relatively smooth, elliptical structure, with a concentrated central bulge. The color is a yellowish-orange, suggesting an older stellar population. There is little indication of spiral arms or active star formation. The galaxy exhibits a high degree of circularity, with no significant elongation or asymmetry detected. There may be some minor disturbances, but not enough to classify it as a merger. Overall, it appears to be a fairly ordinary, well-formed elliptical galaxy.
