The galaxy presents as an edge-on spiral, exhibiting a clear disk structure oriented nearly perpendicular to our line of sight. Dust lanes are apparent as dark, obscuring bands primarily concentrated along the central plane of the disk, bisecting the galaxy's light. A central bulge is visible, appearing more luminous and concentrated than the rest of the disk. The bulge has a smooth, somewhat rounded appearance. The disk shows some evidence of spiral arm structure, though these are tightly wound and difficult to discern distinctly due to the edge-on perspective. There appears to be a slight warp or bending of the galactic disk visible at the edges. Star formation is likely present, given hints of bluer light at the disk's extremities. There is no obvious evidence of a major ongoing merger or strong tidal interactions. Overall, this galaxy is a well-defined spiral galaxy seen from an edge-on viewing angle.
