This galaxy presents an elongated, irregular morphology, suggestive of an ongoing or recent merger event. The primary body appears to be undergoing significant tidal disruption. The central region exhibits a brighter, more concentrated core. Extending from this core are faint, diffuse features, possibly tidal tails or remnants of disrupted galactic structures. Color gradients are apparent, with a shift towards redder hues closer to the core and bluer tones in the outer extremities, possibly indicating variations in stellar populations and dust content. The object's overall structure indicates a dynamic system, potentially in a late stage of interaction with another galaxy.
