This galaxy presents as an edge-on spiral, exhibiting a distinct flattened disk structure. A prominent central bulge is visible, appearing somewhat rounded in shape. Dust lanes are apparent along the plane of the disk, obscuring some of the starlight. Star formation is observed, and is likely occurring throughout the disk. There does not appear to be any significant signs of ongoing mergers or major disturbances to the galaxy's structure. The galaxy's color suggests a population of both young, blue stars and older, redder stars.
