The galaxy presents a clear spiral morphology. It exhibits a prominent central bulge, appearing somewhat elongated. A strong bar feature is visibly traversing the bulge, oriented at roughly the same angle as the bulge elongation. The spiral arms emerge from the ends of the bar.

The arms themselves appear tightly wound, exhibiting a granulated structure, suggestive of numerous star-forming regions along their lengths. The arm structure is relatively symmetrical. The galaxy appears to be undisturbed, with no visible signs of major ongoing merger activity. The arms are blueish in color.
