The observed galaxy presents as an edge-on spiral system, exhibiting a flattened disk morphology. A central bulge is apparent, appearing bright and somewhat rounded. The disk displays a subtle blue tint, suggesting the presence of ongoing star formation, though it appears to be relatively quiescent. The galaxy does not exhibit any obvious signs of recent or ongoing major mergers; it appears as a largely undisturbed system. There may be some slight warping of the galactic disk.
