The galaxy presents a somewhat flocculent spiral structure. Two distinct spiral arms are apparent, displaying a medium winding. A central bulge dominates the core of the galaxy, appearing moderate in size. The galaxy exhibits features indicative of disk characteristics. There is no evidence of a strong bar structure, though the possibility of a weak bar cannot be fully ruled out. No major merger events are readily apparent, though the potential for minor disturbances are present. The color gradient suggests ongoing star formation. 
