This galaxy presents as a disturbed system, possibly undergoing a merger or tidal interaction. A bright, centrally concentrated region dominates the upper portion of the image, exhibiting a relatively smooth morphology with a faint greenish-blue hue. Emanating from this central region, a diffuse, elongated structure extends downward. This extended structure appears less concentrated and displays a bluer color, suggesting the presence of younger stellar populations or enhanced star formation. There appear to be disruptions or distortions within the structure, potentially indicative of tidal features or debris resulting from a gravitational interaction. The overall shape deviates significantly from a regular elliptical or spiral morphology. The system suggests a dynamic and potentially ongoing process shaping its current form.
