The galaxy presents as a diffuse, centrally concentrated object. The core region exhibits a high surface brightness, with the intensity gradually decreasing toward the outer regions. While the central region appears largely featureless, there is a hint of possible structure extending from the central bulge into a disk. There are slight indications of a spiral arm structure within the disk, but these are subtle.

The overall color of the galaxy is slightly red, with a redder central bulge and a bluer disk. There appear to be signs of some minor gravitational disturbance, which could possibly be a tidal tail.
