The galaxy presents as a single object but appears to have two nuclei, indicating a possible ongoing or recent merger event. The larger component exhibits a smoother, more amorphous structure with a somewhat elongated or cigar shape. Its color suggests an older stellar population, likely dominated by redder stars. The smaller component appears more compact and possibly contains younger, bluer stars, as evidenced by its slightly bluer hue. There is some indication of tidal disturbances, which are very slight and diffuse, suggesting a past interaction.
