The galaxy presents as a merging system, with potentially three distinct components engaged in a gravitational interaction. The central region exhibits a relatively smooth morphology, with a concentrated core that appears somewhat rounded in shape. The overall color profile suggests the presence of both older stellar populations, indicated by redder hues, and some regions of ongoing or recent star formation, marked by bluer and greenish tints within the diffuse outskirts of the object. Evident signs of tidal disturbances, possibly indicating an ongoing merger event, are visible, distorting the overall shape of the object and potentially hinting at disturbed internal structure.
