The galaxy displays a generally disk-like morphology. It exhibits a prominent bulge region that appears moderate in size. Faint spiral arm structures are present emanating from the central bulge region, and winding loosely around the galaxy. The galactic disk appears to be oriented close to face-on with respect to our line of sight. The galaxy exhibits a range of colors across its structure. A strong bar feature is possibly present along the central region of the disk. There is no evidence of any major merging activity or major disturbances.
