The galaxy appears to be undergoing a significant merger event. Two distinct luminous cores are visible, suggesting the remnants of two separate galaxies. The overall shape is highly irregular and disturbed, indicative of strong gravitational interactions. A tidal tail or bridge-like structure seems to connect the two cores, showcasing a flow of material between them. The color gradient suggests the presence of both older stellar populations, appearing more reddish/orange, and potentially younger, bluer stars formed as a result of the merger-induced star formation. The general morphology is not clearly spiral or elliptical but is largely dominated by the ongoing merger.
