The galaxy presents as an edge-on spiral. It exhibits a prominent dust lane bisecting its length, obscuring the central bulge and providing a clear demarcation. The bulge appears rounded and well-defined but obscured, with colors tending towards the red end of the spectrum, indicating an older stellar population. The disk shows a faint, elongated structure, with a hint of blueish light along the extremities. Some distortions are apparent, which may imply ongoing or past gravitational interactions. Based on the disk morphology, it is likely a late-type spiral galaxy.
