The galaxy appears as a system undergoing a significant merger. There is not a clear, singular core or nucleus visible. Instead, there are several bright, diffuse clumps of light distributed throughout the galaxy's structure, suggesting multiple centers of stellar density. The overall shape is irregular and disturbed, without any clear spiral arm structure or elliptical form. Some tidal features or distortions are suspected, but the low resolution makes it difficult to ascertain the details. The color is generally yellow to orange. Redder areas are present indicating regions of dust and older stellar populations. This galaxy could potentially be a collection of gas-rich galaxies on a merger trajectory. 
