The galaxy exhibits a morphology consistent with a spiral galaxy. The structure is characterized by a central bulge, which appears somewhat subdued, giving rise to loosely wound spiral arms.

Dust lanes are noticeable within the disk, creating a mottled appearance along the arms. Overall, the galaxy appears to have a flattened disk and a relatively modest bulge component, suggesting a later-type spiral classification.

The color distribution suggests active star formation regions along the spiral arms, which have a bluer tint than the yellowish bulge. The shape of this galaxy is distorted.
