The galaxy presents as a spiral galaxy, viewed at a nearly edge-on angle. A distinct bulge is visible, exhibiting a high surface brightness with a yellowish-white hue, suggesting a relatively older stellar population concentrated toward the galactic center.

The galactic disk is clearly defined, showing a relatively smooth texture. Some dust lane structures are observable along the plane of the disk, exhibiting a faint reddish tinge. 

The outer regions of the disk appear somewhat diffuse, especially at the uppermost part of the image. While the primary morphology suggests an isolated system, subtle irregularities in the disk’s structure, suggest possible minor gravitational interactions or disturbances, as the shape of the galaxy appears distorted on the very edge. The majority of the galaxy appears to be undisturbed however.
