The galaxy presents as a merging system, with two distinct luminous regions. One region appears more concentrated and displays a yellowish-orange hue. The other region is more diffuse, exhibiting a reddish-pink color, suggesting ongoing star formation. A bluish-green component is observed in the region connecting the two luminous areas, potentially indicative of tidal interactions or gas compression due to the ongoing merger. Overall, the system appears highly disturbed, with a complex morphology that deviates significantly from a simple elliptical or spiral structure.
