This galaxy appears to be undergoing a merger, characterized by two distinct luminous regions. The primary region exhibits a yellowish-orange hue, potentially indicating an older stellar population or significant dust obscuration. This region seems to be relatively smooth and rounded in morphology. Positioned below it is a slightly less luminous, more compact region with a whiter hue. The overall structure suggests tidal distortions typical of merging galaxies, although distinct tidal tails are not immediately apparent. The galaxy does not appear to possess a well-defined spiral structure or a prominent disk.
