The galaxy presents as a spiral type, exhibiting a prominent disk structure. Two distinct spiral arms are clearly visible, extending outward from a central bulge. The winding of the spiral arms appears loose. A weak bar structure might be present in the central region. The central bulge appears relatively small to moderate in size compared to the overall disk. The galaxy exhibits a blue hue in the spiral arms. The galaxy does not seem to be undergoing any major merging events or disturbances based on its regular shape, although some minor irregularities are present.
