The observed galaxy presents as a relatively large, elongated structure with a distinct disk-like morphology viewed nearly edge-on. The galactic disk exhibits a clear separation of colors, with a bluer hue along the upper and lower edges, indicative of younger stellar populations and ongoing star formation within the spiral arms. The central bulge appears more concentrated and exhibits a yellowish-orange color, suggesting a higher concentration of older, redder stars. The bulge does not obviously appear boxy or disturbed. The overall light distribution within the disk seems relatively smooth and undisturbed, with no obvious signs of major mergers or significant tidal interactions. The galaxy is relatively luminous. Given the observed color gradients and disk morphology, it is likely a spiral galaxy.
