The galaxy presents as a relatively compact object with a dominant smooth morphology. A subtle disk-like feature appears in the image, however, the smoothness dominates overall. It displays a moderately round shape, leaning toward circular rather than elongated. 

There is no apparent single nucleus, rather a more diffuse central brightness. Evidence suggests the galaxy is undergoing some form of interaction or internal disturbance. There may be ongoing minor interactions as the galaxy also shows indications of possible merger events.
