This galaxy presents as a late-type spiral, viewed nearly edge-on. There is a central bulge that appears relatively small and not particularly luminous. A distinct disk structure can be observed, elongated along its major axis. Patches of blue light indicate regions of active star formation within the disk, which suggests the presence of younger, hotter stars. The galaxy exhibits a smooth texture with some minor disturbances. There does not appear to be a major ongoing merger, although minor interactions cannot be ruled out. Overall, the galaxy is a fairly typical disk galaxy at a modest redshift.
