The galaxy presents as a spiral galaxy, viewed at an angle that is neither face-on nor edge-on. The disk component is evident, displaying prominent spiral arms that appear relatively loosely wound. A bar structure is suggested at the galaxy's core. The bulge is moderately sized, blending smoothly into the disk. Evidences for two dominant spiral arms is present. The morphology suggests ongoing or recent interaction with another galaxy, with some signs of disturbance in the overall structure. The galaxy is actively forming stars.
