This galaxy exhibits a complex morphology. The primary body of the galaxy appears somewhat disturbed, possibly indicating an ongoing or recent interaction. There are two luminous distinct regions. One region is more bluish in color, suggesting the presence of a population of hot, young stars and active star formation. The second region is more red-shifted in color, possibly indicating an older stellar population or significant dust obscuration. The roundness of the body is approximately circular. A tail is visible with signs of a major disturbance. The galaxy's overall structure is not strongly defined, pointing towards a possible transitional state or the aftermath of a significant event.
