The galaxy presents as an edge-on spiral, displaying a flattened disk morphology. A prominent dust lane bisects the galaxy, obscuring the central bulge and contributing to the overall reddish appearance. The bulge appears to be quite prominent and rounded. There is very little evidence of disruption or tidal features which implies it is a fairly isolated galaxy and is not experiencing any major interaction with another galaxy. There appears to be evidence of some flocculent spiral arm structure. The red color suggests an older stellar population throughout the disk.
