The galaxy presents as a diffuse, moderately sized object. It appears to possess a central bulge with an extended, asymmetrical disk. The morphology is somewhat irregular, indicating possible interactions or disturbances. There may be ongoing minor mergers in the vicinity of the galaxy. Evidence of a smooth, featureless component exists, coexisting with indications of spiral arm structures. Patches of concentrated light suggest active star-forming regions, or perhaps superclusters. The outskirts of the galaxy appear to be quite disturbed, and there is a relatively bright light that could be a point of interaction with another smaller object, or something within the galaxy. The light in the disk and bulge is generally uniform, however.
