This galaxy appears to be undergoing a significant interaction, possibly a merger. One component exhibits a smoother, more rounded morphology. The other has a more disturbed structure, appearing more diffuse.

Color variations are apparent within the system. The smoother component displays a yellowish hue, which could indicate an older stellar population or a higher concentration of dust. The disrupted component shows a bluish color, hinting at the presence of younger, hotter stars and active star formation. The galaxy's overall structure is not clearly defined, likely due to the ongoing interaction.
