The galaxy presents as an elongated, edge-on disk galaxy. The central bulge appears bright and concentrated, exhibiting a yellowish hue suggesting an older stellar population with reduced ongoing star formation. Diffuse material extending outwards from the bulge indicates the presence of a galactic disk. This disk seems relatively smooth, lacking prominent spiral arm structures. The outer edges of the disk are fainter and less defined, which suggest a gradual decrease in stellar density moving outwards. Overall, the galaxy seems to be a relatively quiescent system with a notable bulge component and a disk seen nearly edge-on from our line of sight.
