The galaxy exhibits a distinct spiral structure. The spiral arms appear relatively tightly wound. They are somewhat patchy, with discernible areas of enhanced luminosity, suggestive of ongoing star formation regions. The galaxy presents a well-defined central bulge region, but it is not overly dominant. There is evidence of a possible bar structure within the central region. The disk is observed face-on, with a slight inclination making the spiral pattern clearly visible. There are hints of possibly three or more spiral arms. No significant morphological disturbances are seen.
