The object is a galaxy, likely a spiral, observed nearly edge-on. It presents an elongated, disk-like structure. A central bulge is visible, appearing slightly brighter and exhibiting a yellowish hue, suggestive of an older stellar population. The disk shows a gradient in color, with regions closer to the central bulge also appearing yellowish, and the outer regions exhibiting a bluer tint, which is indicative of ongoing star formation.

The disk appears relatively smooth, lacking the distinct spiral arm structures typical of face-on spiral galaxies. There is no obvious indication of a major merger or significant tidal disruption, although minor irregularities cannot be ruled out. The smooth appearance of the disk suggests either a well-mixed stellar population or obscuration by dust, particularly towards the galaxy's mid-plane. Overall, the galaxy presents a regular, relatively undisturbed morphology.