The galaxy presents as a spiral galaxy with a prominent disk structure. It exhibits loosely wound spiral arms which are the dominant feature of the galaxy. The arms display a mottled texture, suggesting active star formation regions interspersed with areas of lower stellar density.

A central bulge is visible, although it appears relatively small in proportion to the overall disk size. There may be evidence of a bar structure.

There is also a merging feature present, with a suggestion of a major disturbance. This could indicate an ongoing or recent interaction with another galaxy.
