The galaxy presents as an edge-on spiral or disk galaxy. A prominent dust lane bisects the galaxy along its major axis, obscuring the central bulge. The bulge appears relatively large and rounded. There is no obvious boxy structure in the bulge region. The disk appears moderately inclined and is observed to have an extended morphology. There are no obvious signs of interaction or major mergers; however, there might be a minor disturbance. Star formation appears to be occurring, but at a relatively low rate. The galaxy exhibits a redder color, suggesting a more evolved stellar population. 
