The galaxy appears as a moderately bright, somewhat flattened spheroid. It exhibits a smooth, diffuse light distribution with a concentration towards the center. The color gradient suggests a possible aging stellar population. While the galaxy doesn't appear to have obvious spiral arms or a bar structure, subtle variations in the light distribution hints at the presence of some internal structure, such as a possible disk or other organized stellar distribution. There is no visually apparent recent interaction with other galaxies or major disturbances to the overall smooth shape. The overall morphology appears to be consistent with an intermediate type galaxy undergoing a relatively low rate of star formation.
