The galaxy presents a discernible spiral structure. The spiral arms are not tightly wound, and exhibit some flocculence. There appears to be some bluing in the arms indicating regions of star formation. A moderate central bulge is observed. No strong bar feature is apparent, though a weak bar is possible. No obvious major distortions or signs of ongoing mergers are immediately apparent, however minor disturbances are possible. The overall morphology suggests a disk-dominated system with ongoing star formation, though perhaps at a modest rate. The galaxy is relatively compact.
