The galaxy appears to be undergoing a merger or significant interaction. Two distinct nuclei are observed, one with a somewhat round morphology and a brighter, more diffuse appearance, and another that is more elongated and less defined. The rounder nucleus exhibits a yellowish-white hue with hints of blue, possibly indicating regions of both older stellar populations and ongoing star formation. The more elongated component displays a yellower color profile. There appears to be a tidal tail, extending outwards in a curved shape, suggesting gravitational disturbance and mass transfer between the components. Overall, the system presents as a disturbed morphology, indicative of a dynamic evolutionary state.
