The observed galaxy presents as a centrally concentrated object with a noticeable degree of smoothness. The primary structure is a somewhat rounded central body with a moderate ellipticity. Evidence suggests a potential merging event or tidal interaction. There is a smaller, secondary structure nearby. The galaxy displays a chromatic gradient, shifting from a bluer hue in the center to a redder tint on the outskirts, suggesting a difference in stellar populations or dust distribution. The overall morphology indicates a system that is either an elliptical galaxy or potentially an ongoing merger that has not fully coalesced.
