The galaxy appears to be an edge-on spiral galaxy of moderate size. A distinct dust lane bisects the galaxy, obscuring the central bulge and indicating significant internal structure. The central bulge is prominent, appearing somewhat boxy or peanut-shaped. The light from the galaxy is more reddish towards the central bulge, with bluer hues concentrated in the outer disk. There is no apparent sign of any major mergers, but there appears to be some minor disturbance as indicated by the warping of the disk. Overall, the galaxy seems to be actively forming stars.
