The galaxy exhibits a disturbed morphology, indicative of an ongoing interaction or merger. Two distinct, bright knots are observed, suggestive of either galactic nuclei or regions of intense star formation triggered by the interaction. The surrounding galactic material displays an irregular and diffuse structure, with faint tidal features that are possibly present, further supporting the merger hypothesis. The color distribution suggests a mix of stellar populations, with redder components likely corresponding to older stars or dust-obscured regions, and bluer components potentially indicating younger, actively star-forming regions. The overall appearance points to a galaxy undergoing significant gravitational and dynamical disruption.
