The galaxy appears to be a spiral galaxy, with a noticeable disk structure. The spiral arms are well-defined and exhibit a predominantly two-armed structure that are moderately wound. There is some evidence of a bar feature across the central bulge. The bulge itself appears to be of moderate size. Some disturbances are seen within the spiral arms. It appears there is a potential small amount of mergers, perhaps a minor interaction or disturbance within the disk of the galaxy. The core of the galaxy demonstrates some evidence of star formation activity.
