The galaxy appears to be in the process of a major merger, with two distinct components evident. The first component exhibits a bluish hue, possibly indicating ongoing or recent star formation. This region also presents a mottled texture, suggestive of patchy dust obscuration or clumpy star formation regions. A slight reddish tint is also present, possibly from the presence of dust or older stellar populations. 

The second component presents a smoother texture with a more yellowish color, suggesting a more evolved stellar population and less active star formation. The overall shape of the combined system appears disturbed and irregular, which supports the presence of a merger. Tidal tails or other merger-related features are not clearly discernible in this image. The morphology suggests a system with a significant stellar mass, in the process of forming a new galaxy as the merger proceeds.
