The galaxy appears to be a spiral galaxy observed nearly edge-on. There is a prominent dust lane bisecting the galaxy's disk, obscuring the central bulge. The bulge, while obscured, seems to be relatively small. Star formation may be occurring, as evidenced by faint blueish regions along the galactic disk. The galaxy displays a notable lack of any significant distortions, tidal tails, or other morphological features indicative of recent major mergers. A slight irregularity is visible on one side of the disk.