The observed galaxy appears as an elongated, disk-shaped structure, indicative of a spiral or lenticular morphology viewed edge-on. A prominent central bulge, exhibiting a yellowish-orange hue, dominates the galaxy's core. The surrounding disk displays a distinct reddish tint towards the outer edges, possibly signifying older stellar populations or dust obscuration. Patches of greenish-blue color are observed within the disk, which could indicate regions of active star formation. There is an absence of any major morphological disturbances or tidal features. The disk appears relatively smooth and well-defined, suggesting it is not currently undergoing a major merger event, though there seems to be a minor disturbance in the upper half of the disk. Overall, the galaxy presents as a well-defined, edge-on disk galaxy with a notable bulge and varying stellar populations or dust content across its structure.
