The galaxy presents as a single, relatively smooth, and centrally concentrated luminous object. It appears to be undergoing a significant interaction, potentially a late-stage merger with another galaxy or a close fly-by with a companion. The structure is elongated with a moderate asymmetry, and it is difficult to discern a distinct disk-like structure. There are two prominent nuclei that are surrounded by what looks like a tidal tail. The color gradients suggest relatively older stellar populations throughout. The galaxy appears to be relatively quiescent, with a low star formation rate.
