The galaxy appears as a yellowish, diffuse object with a complex morphology. There are at least three distinct, bright concentrations of light embedded within a more extended, fainter halo. These concentrations suggest the presence of multiple nuclei or regions of intense star formation. The overall shape deviates significantly from a regular elliptical or spiral structure. The light distribution seems disturbed, potentially indicative of ongoing or recent merger activity. The smooth component accounts for a large fraction of its total luminosity. There is evidence that the object is undergoing a merger.