The galaxy appears to be a spiral galaxy, viewed at an angle between face-on and edge-on. It exhibits a central bulge that appears relatively prominent and concentrated. Spiral arms are visible and appear tightly wound, and based on the arms visible there are likely two or three of them. There appears to be a presence of more prominent star formation within the galaxy. There is a slight degree of dust lane obscuration observed, particularly along the near side of the disk. The galaxy displays a generally smooth and undisturbed morphology, showing no obvious signs of ongoing major mergers or tidal interactions.
