The galaxy presents as an edge-on spiral galaxy. It exhibits a pronounced dust lane bisecting the galaxy along its major axis, characteristic of spiral galaxies viewed from this orientation. The central bulge appears relatively small, with a mostly unnoticable bulge. The galactic disk shows a smooth light distribution, with a lack of any obvious flocculent or grand design spiral arm structures. The galaxy demonstrates a blue hue, which is indicative of moderate star formation occuring. There are no signs of strong tidal distortions or close companions, suggesting an isolated evolutionary path, although there are small signs of some minor distrubances within the disk itself.
