The galaxy presents as a spiral type with a clearly visible disk structure. Evident spiral arms emanate from a central bulge. The arms appear loosely wound and patchy, suggesting ongoing star formation within them. Patches of bluer light are noted within the arms, indicating the presence of younger, hotter stars. The central bulge exhibits a more concentrated, yellowish hue, possibly indicating an older stellar population. The galaxy is not perfectly symmetrical, with some asymmetry in the arm structure, which could indicate a past interaction. There may be a possible minor disturbance to the morphology, but no obvious signs of a major merger are seen.
