This galaxy presents a complex morphology, appearing as a spiral galaxy viewed at a significant inclination relative to our line of sight. The disk is prominent, exhibiting a non-uniform distribution of luminosity across its surface. Spiral arm structures are visible, though somewhat diffuse, suggesting a flocculent or grand-design structure.

A central bulge is present, but it appears relatively subdued compared to the disk component. The bulge does not dominate the overall light profile.

There is evidence of a bar-like structure crossing the central region of the galaxy. Patches of enhanced blue emission are scattered throughout the disk, indicative of ongoing star formation within the spiral arms.

The galaxy displays some signs of interaction or disturbance. There are some irregularities in the spiral arm structure and a slightly disturbed overall shape. This may indicate a minor interaction or merging event in its recent past.
