The galaxy presents a disk-like structure. Prominent spiral arms are visible, exhibiting a morphology consisting of two tightly wound arms, which originate close to the central region. The core is a bright, condensed bulge. Coloration suggests ongoing star formation, evidenced by the blue hues in the spiral arms. There is a weak bar running through the center of the galaxy. There is no obvious evidence of any major disturbances, but the spiral structure is not fully symmetrical.