The galaxy exhibits a complex morphology suggestive of an ongoing merger event. Two primary components are readily discernible: a larger, diffuse component appearing relatively smooth, and a smaller, more compact component. The larger component displays a slightly elongated shape. The smaller component appears bluer in color, possibly indicating younger stellar populations and ongoing star formation. The overall light distribution is not symmetrical, with the peaks of emission offset from what would be expected for a single, relaxed system. There is an additional bluer patch below these structures, connected with a faint stellar bridge. The galaxy's integrated color is moderately red, suggesting an intermediate age and/or dust content. The smoothness of the primary component suggests it may evolve into an elliptical galaxy after the merger has completed.
