The galaxy presents an elongated, edge-on morphology. A distinct dust lane appears to bisect the galaxy's structure horizontally, indicating a significant concentration of interstellar dust within the galactic plane. The central bulge exhibits a relatively smooth appearance with a yellowish hue, suggesting an older stellar population. Fainter blue emissions extend from the mid-plane, tracing the galactic disk. The disk appears thin and flattened, characteristic of spiral galaxies observed edge-on. There does not appear to be a central bar, but the bulge structure is difficult to resolve at this viewing angle. There is a possible smooth halo enveloping the galactic disk.
