The galaxy presents as a spiral type, viewed at a slight angle to edge-on, but significantly closer to face-on. Faint, tightly wound spiral arms are discernable, although the exact number is somewhat difficult to ascertain. The arms appear somewhat patchy in nature. The central bulge is relatively small and not particularly luminous. A bar structure appears present across the central region. There may be some signs of minor tidal disturbances, suggesting the possibility of past interactions. The galaxy is likely undergoing moderate to low levels of star formation.
