The galaxy presents as a system undergoing a significant merger. It appears to be interacting with at least one other galaxy, possibly two, resulting in a disturbed morphology. A central, relatively bright region is observed, with what appear to be tidal tails or extended features emanating from it. These features display a lower surface brightness and suggest gravitational interactions are actively reshaping the system. The color profile of the central region appears slightly redder, possibly indicating an older stellar population or increased dust obscuration. The extended features show a bluer tint, hinting at more recent star formation within these regions likely triggered by the ongoing merger event. Overall, the galaxy exhibits signs of significant dynamical activity and morphological irregularity.
