The galaxy appears to be undergoing a merger event. The system presents as two distinct luminous centers, potentially representing the cores of the original galaxies involved. The larger of the two cores exhibits a bluer color, indicative of a population of younger, hotter stars and ongoing star formation. The second core displays a more yellowish hue, possibly representing an older stellar population. Diffuse light surrounds both cores. The overall morphology suggests gravitational interaction and tidal forces are actively reshaping the galaxy's structure. There is evidence of disturbance in the form of a plume or tail extending from one of the merging components.
