The galaxy presents as a disturbed system, likely undergoing a merger or interaction. Two distinct, relatively bright cores are visible, with each core surrounded by diffuse, extended emission. The color of the cores appears yellowish-white, potentially indicating an older stellar population. The outer regions show hints of tidal features and irregular structure, suggesting gravitational disruption. There is a color gradient visible, with bluer colors, particularly toward the edges. This could be indicative of more recent star formation.
