The galaxy presents as a relatively face-on spiral, exhibiting a central bulge. The spiral arms are tightly wound, giving the galaxy a flocculent appearance. A slight asymmetry is observed in the distribution of the spiral arms, with a greater concentration on one side. There are numerous spiral arms and the galaxy appears to have a central bar structure. The bulge appears small relative to the galactic disk. The overall color suggests a relatively high rate of star formation. The galaxy's shape is more elliptical than circular. There are no signs of any major disturbances.
