The galaxy presents as a disturbed system, exhibiting signs of an ongoing or recent merger event. Morphologically, it appears centrally concentrated with a smooth, albeit irregular, light distribution. A distinct feature is the presence of multiple nuclei, suggesting that the system is composed of at least two galaxies in the process of coalescing. The color gradient observed indicates variations in stellar populations and dust content across the galaxy. There is likely substantial mixing of stellar material and gas clouds throughout the merging system. Tidal features, such as faint extensions or streams, are not clearly visible, which could be due to their low surface brightness, suggesting they are not pronounced or are difficult to observe at the given depth of the image. Overall, it displays an advanced stage of interaction, indicative of significant gravitational disruption and dynamical evolution.
