The galaxy presents a complex morphology suggestive of an ongoing or recent merger event. There is a dominant, relatively bright and compact core, exhibiting a bluish hue. Adjacent to this is a larger, more diffuse component with a yellowish tinge. This second component is less centrally concentrated and appears to be tidally distorted. The overall shape of the galaxy is irregular, lacking any clear spiral arm structure or elliptical symmetry. There appears to be a possible tidal tail extending outwards, indicating gravitational interaction. Patches of varying color intensity, and overall irregular morphology suggests enhanced star formation and the presence of dust lanes, further indicating the dynamic processes associated with a merger. 
