The galaxy presents as a spiral galaxy with a moderate inclination relative to our line of sight. Two symmetric spiral arms emerge from the central bulge. The arms are tightly wound and can be traced for a distance of roughly 6 kpc, and feature regions of active star formation along their length. The bulge is relatively small. The inner regions of the galaxy, closest to the bulge, appear smoother and more uniform in color compared to the outer spiral arms. There is a possible bar structure partially visible in the central region of the galaxy. Based on visual disturbances, it may be undergoing or have recently undergone a merger event.
