The galaxy presents as a system undergoing a significant merger. A larger, more diffuse component dominates the visual structure, exhibiting a smoother morphology with a slight central concentration of light. This component displays a faint, blueish hue, possibly indicative of recent or ongoing star formation. Interacting with the primary galaxy is a smaller, more compact component, that appears yellower. The irregular shape and disrupted light distribution suggests tidal interactions are at play. The overall system size is significant, spanning a considerable angular extent, indicating that the tidal interactions may be strong.
