The object appears to be a spiral galaxy, observed nearly edge-on. It exhibits a somewhat elongated, cigar-shaped morphology. The central bulge is not particularly prominent, and there is faint evidence of a disk structure extending outward. The color gradient suggests a relatively older stellar population, possibly indicating a lower rate of star formation. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or significant tidal interactions. There may be a slight asymmetry in the disk structure.
