The galaxy presents as a moderately luminous, disk-shaped system, viewed nearly edge-on. A distinct dust lane is not easily observed, but is implied in the lack of light around the central bulge.

The radial color gradient shows a distinct trend, with the central regions appearing yellower, possibly indicating an older stellar population. The disk regions appear bluer, hinting at ongoing or recent star formation. There seems to be an object at one side of the galaxy that looks like a merger or companion galaxy. There are no obvious signs of grand-design spiral arms. The overall morphology suggests a relatively massive galaxy experiencing some level of interaction with another galaxy. Star formation rate appears to be quite low.
