The galaxy presents as a face-on spiral with a prominent central bulge exhibiting a yellowish hue, suggestive of an older stellar population. The spiral arms are loosely wound and traced by regions of bluer light indicative of ongoing star formation. Two dominant spiral arms appear to originate near the central bulge. No signs of major mergers are obviously disrupting the symmetry of the disk, although there may be some minor tidal disturbances visible. The stellar mass is estimated to be high, and moderate star formation is ongoing. The shape of the spiral arms suggest a barred morphology may be present. The galaxy is not edge-on.
