The object presents as a spiral galaxy. It exhibits a disk morphology viewed at an oblique angle, not quite edge-on. Two distinct spiral arms appear to emanate from a central bulge, displaying a grand design structure. The arms are loosely wound, and appear to contain clumpy regions that suggest areas of active star formation. The central bulge appears relatively large and bright, indicating a significant concentration of stars. The galaxy appears to lack a prominent bar structure. There is no obvious evidence of major galactic interactions or mergers. The general color of the galaxy suggests the presence of both older stellar populations and younger, bluer stars within the spiral arms. The light distribution indicates this galaxy is moderately large.
