The galaxy presents as a flattened, disk-like structure with a prominent central bulge. The overall color is a warm, yellowish-orange, suggesting an older stellar population dominates the light output. A faint, but discernible, dust lane is possibly present along the major axis. The spiral arm structure is not well-defined, appearing more flocculent than grand design. The galaxy is significantly tilted with respect to the line of sight, revealing an edge-on perspective that obscures some of its internal features. The central bulge exhibits a smoother texture than the outer disk, indicative of a higher stellar density. There is a weak hint of ongoing star formation activity. The overall morphology suggests a galaxy that is possibly an intermediate spiral or a lenticular galaxy.
