The galaxy presents a disk-like structure with a noticeable central bulge. Spiral arms are clearly visible, exhibiting a tightly wound morphology. The bulge appears to be moderate in size relative to the overall disk. There is evidence of a bar-like structure spanning across the central region of the galaxy. The disk's color suggests active star formation, with the spiral arms displaying a bluer hue compared to the yellowish-white bulge. The arms are somewhat flocculent in appearance, lacking a grand design. No major signs of ongoing mergers, or significant disturbances are immediately apparent from its morphology, although there may be some indications of minor disturbances within the arms.
