The observed galaxy exhibits a distinct edge-on morphology, presenting as a flattened, elongated structure. A central bulge region is evident, displaying a concentration of older stellar populations, indicated by the yellowish-orange hue. The disk component appears thin and elongated, with some indication of dust lanes obscuring the light from stars within. The galaxy does not show any signs of ongoing major mergers or significant tidal disturbances, although the presence of minor internal distortions cannot be entirely ruled out at this resolution. Overall, the galaxy appears to be a relatively quiescent disk galaxy with a prominent bulge and a stable, well-defined structure.
