The object presents as a spiral galaxy viewed at an oblique angle. A prominent central bulge dominates the core, exhibiting a smooth, yellowish-white glow. The galaxy disk displays a discernible spiral structure, with arms that appear somewhat tightly wound. There seems to be 2 main spiral arms. These spiral arms show subtle variations in color, with hints of bluer regions suggestive of younger stellar populations. The image suggests a possible bar structure extending through the central region. There are no apparent signs of a major merger or significant tidal distortions within the galaxy's structure, though there is a slightly disturbed morphology, implying potential minor gravitational interactions.
