The galaxy presents as a relatively smooth, centrally concentrated object. It appears to be a disk galaxy, possibly a lenticular or early spiral type, where most of the light seems to emanate from the central bulge, with light that gradually fades out with the disk. The overall color is fairly blue-white, suggesting the presence of a relatively young stellar population and recent star formation. There is a slight hint of elongation, but the structure appears mostly relaxed with no strong signs of major disturbances or ongoing mergers, although there is some subtle fuzziness in the disk. The light is most likely due to it being a moderate mass galaxy.
