This galaxy appears to be an interacting system, consisting of two distinct components. The larger component exhibits a relatively amorphous morphology with a centrally concentrated light profile. A fainter, less defined structure extends outward from the central region. The smaller component presents a more compact and distinct form, suggestive of a separate galactic entity. There appears to be some tidal disruption or distortion visible in the region connecting the two components, indicating gravitational interaction. The overall color of the system suggests a mix of stellar populations, with bluer regions indicating younger stars and ongoing star formation, and redder regions potentially indicating older stellar populations or dust obscuration. Evidence of disturbances in the overall structure might indicate a minor or major merger is occurring.
