The galaxy presents an apparent morphology suggesting an ongoing or recent interaction, potentially a merger. There are at least two distinct, bright components. The larger, more diffuse component appears ellipsoidal. This main component exhibits a smooth light distribution with a yellowish-red hue. The smaller component presents a more elongated form, possibly indicating tidal disruption. The overall system demonstrates signs of morphological disturbance, deviating from a simple, relaxed structure. The system is also fairly large.
