The galaxy presents as a complex system, likely undergoing a significant interaction or merger. It exhibits a disturbed morphology, deviating substantially from a regular elliptical or spiral structure. Several distinct, yet interconnected, luminous regions are apparent, suggesting multiple galactic cores or intense star-forming knots. The overall shape is elongated, with a hint of tidal tails extending outwards, further supporting the hypothesis of an ongoing gravitational interaction. The central region shows a mixture of colors, with indications of both older stellar populations (redder hues) and ongoing star formation (bluer hues). Overall, the galaxy appears to be a system characterized by strong gravitational disturbances and active star formation, likely triggered by the interaction or merger event.
