The observed galaxy presents as a highly inclined, edge-on spiral system. A prominent central bulge, appearing yellowish, dominates the galaxy's structure, suggesting a significant population of older stars concentrated towards the core. Faint, diffuse disk is visible extending outwards from the bulge, exhibiting a bluer tint indicative of more recent star formation. The disk appears relatively smooth with no immediately discernible spiral arm structure. The galaxy appears relatively undisturbed, showing no obvious signs of major mergers or tidal interactions.
