The observed galaxy presents as a spiral galaxy, with the majority of classifications indicating a spiral structure. The galaxy is oriented somewhat edge-on, but the spiral arms are still visible. Predominantly, the classifications suggests two main arms winding outwards in a regular manner. The winding of these arms is described as medium. There is a bar-like structure present within the central bulge; tending to the weaker side.

The central bulge appears moderate in size relative to the disk and is notably brighter and yellower than the surrounding spiral arms, indicating an older stellar population. Some features indicating a minor disturbance are present; not presenting any major disruptions in the overall morphology. The smoothness of the galaxy is low, with distinct, disk-like features.