This galaxy exhibits a moderately inclined disk-like morphology. There is evidence of both a smooth component and a more featured, potentially spiral structure within the disk. The central bulge appears prominent and relatively bright. The overall color profile suggests ongoing star formation within the disk, although the disk exhibits some areas of differing color, which could indicate areas with different densities of gas and dust. There is no compelling evidence of a major merger, but subtle disturbances within the disk hint at possible minor interactions or internal instabilities.
