The galaxy presents as a spiral type, observed at a significant angle from edge-on. The central bulge appears prominent and exhibits a yellowish-white hue, suggesting an older stellar population. Faint spiral arms extend from the central bulge. The arms show areas of bluer light indicative of younger, hotter stars and some dust lanes. The overall structure seems relatively undisturbed with no obvious signs of major mergers. The disk appears to be smooth with the presence of some features. The light from the galaxy is quite red in color and shows it is a quite massive galaxy with a low star formation rate.
