The observed galaxy presents as a spiral galaxy viewed nearly edge-on. A prominent central bulge with a yellowish hue dominates the galaxy's core, indicating a population of older stars. The galactic disk appears as a flattened structure with a bluish tint, suggesting the presence of younger stars and ongoing star formation. Dust lanes are subtly visible along the disk, obscuring some of the starlight. One side of the disk appears to be much brighter than the other, perhaps due to a higher concentration of star forming regions or to it simply being closer to the observer. The galaxy appears relatively undisturbed, with no significant signs of recent major mergers or tidal interactions, though there is a smaller object nearby which may be related. The overall color profile indicates moderate star formation activity within the galaxy.
