The galaxy presents a distinct spiral structure. The spiral arms appear open and loosely wound. Two dominant arms are discernible, tracing a somewhat irregular path from the central region outwards. The central bulge exhibits a moderate size, displaying a yellowish hue, which may indicate an older stellar population. Patches of bluer light are observed along the spiral arms, indicative of active star formation regions. The galaxy shows no clear signs of a significant bar structure, with only a slight elongation possibly indicative of a weak bar. There are no obvious signs of a major merger event. Some minor tidal disturbances or asymmetries could be present, warranting further investigation.