The galaxy presents a complex morphology, appearing as a central, relatively bright core surrounded by a more diffuse, elongated structure. The core region exhibits a bluish hue, possibly indicative of ongoing or recent star formation activity involving hotter, younger stars. The extended, less luminous component displays a more reddish color, which might suggest a population of older, cooler stars or the presence of dust obscuring bluer light. There are signs of tidal disruption, potentially indicative of an ongoing or recent merger event. A faint tail can be discerned emanating from the main body, perhaps a stream of stars or gas pulled away from the galaxy due to gravitational interaction. Overall, the galaxy displays features suggesting a disturbed morphology and a complex evolutionary history.
