The galaxy appears to be undergoing a significant interaction or merger. There are two distinct, bright central components. The primary component is slightly diffuse and elongated. A secondary component is more compact and possesses a yellowish hue. A faint tidal tail is also apparent emanating from the primary central component, indicating gravitational disruption. The overall morphology suggests a relatively late-stage merger, with the two components approaching coalescence. The galaxy shows evidence of ongoing star formation. Its overall shape exhibits characteristics that range from round to disturbed. 
