The galaxy appears to be an elliptical galaxy, with a smooth, centrally concentrated light profile. It exhibits a yellowish hue, suggestive of an older stellar population. The galaxy is moderately elongated, displaying an axial ratio of approximately 0.7. There is no discernable spiral structure or dust lanes, supporting the classification as an elliptical galaxy. The outer regions fade gradually, indicating a lack of distinct boundaries. The overall appearance suggests a galaxy that has largely completed its star formation, composed predominantly of older, redder stars.
