The galaxy presents an irregular morphology, indicative of a system undergoing significant gravitational interaction, possibly a merger. Two primary luminous regions are discernible, one more centrally concentrated and another more diffuse. The concentrated region exhibits a reddish hue, suggestive of an older stellar population or significant dust obscuration. The diffuse region displays a more complex coloration with tinges of green, potentially indicating ongoing star formation. A faint tail or bridge-like structure appears to connect the two regions, possibly tidal debris resulting from the interaction. Overall, the system's structure is disturbed, lacking a well-defined disk or spheroidal component. This suggests it is in a late stage of a merger event, with significant disruption to its original morphology.
