The galaxy presents as a disk galaxy, viewed at a high inclination angle, close to edge-on. There is a central bulge, appearing yellowish-white, that dominates the inner region, suggesting an older stellar population. The disk extending outwards is less defined with light smearing across it, but appears to contain a mix of younger, bluer stars and older, redder stars. There does not appear to be a prominent dust lane bisecting the galaxy. The morphology appears relatively undisturbed, showing no signs of tidal tails or other major distortions indicative of recent mergers. The galaxy's apparent angular size is moderate.
