This galaxy appears to be undergoing a significant interaction or merger. The primary body shows a disturbed morphology, with evidence of tidal features extending outwards, particularly on its left side. These features exhibit a bluer color, suggestive of ongoing or recent star formation. 

Within the main body of the galaxy, there are multiple, brighter clumps. These could represent either the original nuclei of merging galaxies or regions of intense star formation triggered by the interaction. These clumps appear more yellow, implying an older stellar population or dust obscuration.

Overall, the galaxy does not present a smooth, elliptical appearance; the overall structure appears irregular, supporting the interaction hypothesis. There is an indication of moderate dust content, considering the reddening effects observed within the core of the galaxy. The galaxy appears relatively compact.
