The galaxy presents a morphology indicative of an ongoing or recent interaction. It appears as two distinct, luminous components separated by a noticeable gap, suggesting a possible merger event. One component displays a more diffuse, elongated structure, appearing somewhat irregular. The other is more compact and circular, exhibiting a bright, concentrated core. There is a color gradient between the two, with the elongated structure appearing bluer and the round structure appearing yellower. There may be faint tidal features or distortions visible, indicating gravitational disturbances.
