The galaxy presents as a well-defined spiral, exhibiting a prominent, moderately sized bulge. This central region displays a yellow-orange hue, suggesting an older stellar population.

The spiral arms are tightly wound, extending outwards from the central bulge. The arms display prominent HII regions, visible as blue clumps along the spiral arms, and a blueish disk.

The disk of the galaxy appears slightly inclined relative to our line of sight. There also appears to be another less developed arm reaching away from the galaxy. 

The galaxy appears to be undergoing a merger, which has made it appear amorphous, although there is a very clear spiral structure.