The galaxy appears to be undergoing a significant interaction, possibly a merger. It is composed of at least two distinct components. The first is a centrally concentrated, relatively smooth and rounded component exhibiting a yellowish-orange hue. This suggests a population of older stars dominating this region. The second component appears more diffuse and exhibits a bluer color, hinting at regions of ongoing star formation. There are disturbances present in the disk, indicating that it is not in equilibrium. This suggests a recent interaction or merger.