The observed galaxy appears to be in a late-stage merging process, potentially involving two distinct galactic nuclei. Each nucleus is characterized by a bright, relatively compact central region exhibiting a bluish hue, suggestive of active star formation possibly triggered by the ongoing interaction. There is a faint yellowish-orange glow between the two nuclei, indicating tidal material or a pre-existing galactic disk distorted by the gravitational interaction. The overall morphology is disturbed with no clear spiral or elliptical structure readily apparent. Minor features or irregularities within the galactic structure are not easily discernible due to their subtle nature. There may be some evidence of minor tidal features or distortions, but without more depth of image, its difficult to say for sure.
