The galaxy appears to be undergoing a significant interaction, possibly a merger. There is a bright, relatively compact central region with a bluish hue, suggestive of a population of younger, hotter stars. Adjacent to this, there's a more diffuse, elongated component with a yellower color, possibly indicating an older stellar population or dust obscuration. The overall morphology is irregular, lacking any clear spiral arms or elliptical structure, which supports the possibility of a disturbed system. There is a distinct disruption to the shape with a less clear extension of the galaxy. It is challenging to discern if this disruption is due to tidal effects or internal processes within the galaxy.
