The galaxy appears to be undergoing a significant merger event. Its morphology is highly disturbed, showing multiple distinct luminous clumps and tidal features. The primary body of the galaxy exhibits a somewhat elongated shape, but with substantial irregularities. There is evidence of potential spiral arm remnants or tidal tails extending outwards. The color distribution is complex, with a central blue-white concentration, likely indicating a region of active star formation, and surrounding areas exhibiting a redder hue, possibly associated with older stellar populations or dust. The overall appearance suggests a system in the midst of a dynamic and disruptive interaction. There appears to be multiple galactic cores visible within the merging system.