The galaxy presents as a diffuse object with an irregular morphology. The central region exhibits a concentrated, albeit somewhat indistinct, structure with a yellowish hue. Extending outwards from this core, there are fainter, seemingly disjointed features, potentially indicative of tidal disturbances. The light distribution suggests a system undergoing some form of interaction or disturbance, with the possibility of merger activity contributing to its present form. The overall color profile indicates a substantial population of older stars, with a possible localized burst of recent star formation contributing to the patchy yellowish regions. The galaxy's shape tends towards a somewhat rounded appearance, though this is significantly disrupted by its features. Evidence indicates a system with ongoing or recent dynamic processes.
