The galaxy presents as a spiral type, with moderately defined spiral arms. The arms appear somewhat flocculent, exhibiting a patchy structure. Bluer regions are observed along the outer arms, possibly indicating areas of active star formation. The central bulge region is prominent and appears yellowish, suggesting a population of older stars. The bulge appears small relative to the overall disk size. The galaxy shows evidence of minor disturbance or possible interaction, as the disk shows some asymmetry. A weak bar structure may be present. Overall, the galaxy appears to be a disk-dominated spiral, exhibiting ongoing star formation.
