The galaxy appears to be undergoing a major merger. There are two distinct, bright nuclei visible, each with a somewhat irregular morphology. Both galactic nuclei are similar in brightness, and each exhibits a concentrated central luminosity, which is indicated by the white and blue colors. The distribution of light around each nucleus appears diffuse and somewhat amorphous, rather than conforming to a clear spiral or elliptical structure. There are faint indications of tidal tails or bridges of material extending between the two nuclei. This suggests strong gravitational interaction and potential disruption of the pre-merger galactic structures. The overall color profile is fairly uniform across the merger system, with a slight bluer hue, which may indicate recent or ongoing star formation activity. The image suggests a dynamic system in the later stages of a galactic merger event.
