The galaxy appears to be in the process of merging, displaying a disturbed morphology. Two distinct galactic nuclei are visible, each exhibiting a concentrated luminosity. The larger nucleus shows a more diffuse, yellowish hue, while the smaller nucleus appears more compact with a warmer color. A faint bridge of material seems to connect the two nuclei, indicating gravitational interaction. The overall shape is elongated and irregular, deviating significantly from a simple elliptical or spiral structure. There is evidence of tidal tails or debris extending from the main body, supporting the ongoing merger event. The system exhibits a relatively smooth appearance, although there is a hint of irregular structure, potentially indicative of active star formation within the interacting components. The object shows a moderate redshift, placing it at a significant cosmological distance.
