The galaxy presents as a spiral type, with a notable disk structure. The spiral arms are somewhat flocculent, displaying a patchy distribution of star formation. A central bulge is visible, though it appears relatively small in proportion to the overall disk size. The galaxy exhibits a moderate inclination relative to our line of sight. Evidence of some interactions with a minor disturbance may be seen through asymmetries in the spiral arm structure, potentially influenced by ongoing gravitational interactions. The colours suggest on-going star formation.
