The galaxy presents a disturbed morphology, indicative of an ongoing or recent merger event. The central region appears diffuse and asymmetrical, lacking a well-defined nucleus. Faint tidal tails or streams extend outwards, suggesting gravitational interaction with another galaxy. The overall color is slightly reddish, which may indicate an older stellar population or the presence of dust obscuration. The galaxy's light is dispersed over a moderate area of the sky, neither appearing particularly compact nor highly extended. Patches of bluer light may indicate recent star formation in certain regions. The asymmetry and disrupted features are the most prominent characteristics, pointing towards significant gravitational disturbance in the galaxy's recent history.
