The galaxy presents as a merging system, likely in the late stages. Two distinct, bright nuclei are visible, exhibiting a yellowish-orange hue, indicative of an older stellar population. There is an apparent gravitational interaction disrupting their morphology. Faint tidal features, plumes or tails are not distinctly visible, suggesting a smoother, less chaotic merging process or a considerable distance obscuring such details. The overall shape approximates a rounded, singular entity, a nearly complete merger. The system exhibits a relatively smooth appearance, implying that active star formation is not prominent at the visible wavelengths. The galaxy is a substantial object, considering its luminosity and redshift.
