The galaxy presents as a spiral galaxy viewed at an angle. It exhibits a central bulge, although not particularly prominent. A bar feature appears to extend across the bulge region. Two distinct spiral arms wind loosely from the central region. The spiral arms show some patchiness, possibly indicating regions of active star formation. The galaxy is not undergoing any major merging events, although it is possible there is a minor disturbance from a possible small merger event. The galaxy is not viewed edge-on. The overall color suggests the presence of both older stellar populations in the bulge and younger, bluer stars in the arms. The spiral winding is loose. The galaxy shows a mostly smooth disk with some features in the arms.
