The galaxy presents a complex morphology. The primary structure appears to be a spiral galaxy, albeit somewhat disturbed. It exhibits a central bulge, with a prominent disk extending outwards. The disk structure appears irregular and exhibits hints of spiral arm features, however these are asymmetric.

One notable feature is a bright, unresolved blue object superimposed on one of the arms. The color suggests ongoing star formation or potentially an active galactic nucleus. The overall color of the galaxy tends towards the redder end of the spectrum, with a yellow-orange hue dominating the bulge and inner regions of the disk, implying an older stellar population.

There are visual indications of possible tidal disturbances or interactions with other galaxies. One can see faint streams of material extending away from the primary disk, this indicates possible merger activity.
