The galaxy presents as a disturbed system, exhibiting characteristics suggestive of a possible ongoing or recent merger event. The morphology is not clearly elliptical or spiral, indicating a possible interaction. Two distinct luminosity peaks are observed, possibly indicating two merging galaxies. The galaxy's overall color profile appears moderately red-shifted. The image shows a diffuse outer halo, suggesting a gravitationally disturbed system. Some faint tidal features may be visible on close inspection, supporting the merger hypothesis. Overall, the morphology suggests a dynamically active system undergoing a merger or recent interaction. 
