The galaxy appears to be an edge-on spiral galaxy. It exhibits a prominent, elongated disk. The bulge appears relatively rounded and centrally concentrated. There is no clear evidence of a bar structure. The galaxy shows a fairly smooth structure, with no readily apparent strong tidal features or major disturbances indicative of a recent merger. However, there is a hint of a minor disturbance. Based on the estimated star formation rate, the galaxy is actively forming stars. The dust lane obscuring the disk appears somewhat patchy.
