The galaxy appears as a relatively small, somewhat faint object. The morphology suggests a disk galaxy, though not highly pronounced. It has a somewhat smooth appearance with only a very slight indication of spiral arms. The core region appears brighter and slightly more blue-shifted than the outer disk, suggesting the presence of a population of younger, hotter stars towards the galaxy's center. The disk itself exhibits a reddish hue suggesting there are older stars that compose the galactic disk, with ongoing star formation at a low rate. There's also the possibility that there is ongoing or past merger activity.
