The galaxy appears to be undergoing a significant interaction or merger. It presents a somewhat irregular morphology, with two distinct, bright concentrations of light suggesting either two nuclei or a disrupted core and a separate, dense region of star formation. A faint, diffuse halo surrounds these central components, extending unevenly and displaying tidal features, possibly streams of stars and gas being pulled away from the main body. The overall color is yellowish-orange, indicative of an older stellar population, although there might be pockets of younger, bluer stars contributing to the overall light. The disturbed morphology suggests a dynamic event, possibly a recent or ongoing merger disrupting the galaxy's original structure.
