The galaxy presents as a disturbed system, potentially in the late stages of a major merger. There are two distinct luminous components connected by a faint bridge of material. One component appears more compact and slightly elongated. The other component exhibits a more diffuse morphology, seemingly in the process of tidal disruption. The color gradient across the system suggests variations in stellar populations, with regions exhibiting a higher concentration of older, redder stars, while other areas show evidence of younger, bluer stellar populations. The overall system is relatively compact, with a noticeable departure from a smooth, elliptical profile. There are also some signs of minor tidal features extending from the main body, indicating ongoing gravitational interactions.
