The observed galaxy presents as a spatially extended, disk-shaped system viewed nearly edge-on. A prominent central bulge appears relatively smooth and slightly elongated, exhibiting a yellowish hue, potentially indicative of an older stellar population. Extending outwards from the central bulge, the galactic disk exhibits a flattened morphology, characterized by a bluer color gradient, suggesting the presence of ongoing star formation within its spiral arms or disk structure. The disk appears relatively undisturbed, without any major signs of tidal interactions or recent mergers. Faint dust lanes are suspected within the disk, partially obscuring the starlight from the bulge. The overall impression is of a mature spiral or lenticular galaxy at a considerable distance, with a disk that is rich in gas and dust, resulting in new stellar nurseries.
