The observed galaxy presents as an edge-on spiral, with a prominent central bulge. The bulge exhibits a smooth, rounded morphology. Dust lanes are likely present within the disk, contributing to the mottled appearance and obscuration of light. Based on the apparent color gradient, the bulge appears to consist of a population of older stars compared to the disk. The disk is relatively thin and extended, and the galaxy shows no obvious signs of major mergers or significant tidal disturbances. The overall structure suggests a relatively evolved spiral galaxy, seen at a considerable distance. There is a hint of structure within the disk, potentially indicating the presence of spiral arms, though these are not clearly defined. Overall, the light from this galaxy is dominated by longer wavelengths.
