The galaxy exhibits a prominent spiral structure. Two well-defined spiral arms appear to emanate from a central bulge, displaying a medium winding. The bulge appears relatively small and is yellowish in color, suggesting an older stellar population. The spiral arms exhibit a bluer hue, indicative of ongoing star formation. The disk of the galaxy is not viewed edge-on. There is no major morphological disturbance suggesting a recent merger event. The galaxy appears to be a late-type spiral galaxy. 
