The galaxy appears to be a spiral galaxy viewed nearly edge-on. There is a central bulge that seems relatively small and not very luminous. The disk is clearly visible, with a noticeable dust lane running along its length, bisecting the galaxy. The light from the disk is relatively uniform, showing only subtle hints of spiral arm structure. There is no clear indication of a recent major merger or strong tidal disturbance affecting the galaxy's morphology. The overall color suggests a galaxy with a modest amount of recent star formation, but likely not a very high star formation rate.