The galaxy presents as a spiral, observed at a high inclination. The bulge component appears relatively small and not particularly prominent. The disk structure is clearly visible, exhibiting spiral arm morphology with a clumpy texture. The galaxy presents a noticeable asymmetry, with one side appearing somewhat more extended than the other. There is evidence of on-going star formation activity, particularly along the spiral arms which appear to be well defined. The color of the spiral arms is mostly a blue-ish white, indicating the presence of young stars, particularly towards the extremities.
