This galaxy exhibits a morphology suggestive of a merging system. Two distinct, luminous cores are observed, appearing almost spheroidal in shape. The overall color gradient indicates a population of older stars, with a redder hue dominating the visual appearance. There's evidence of tidal distortion, with faint, extended arms of galactic material emanating from both cores, particularly towards the lower region. The system displays a compact structure, implying a relatively advanced stage of merging. Further analysis is needed to determine the precise physical characteristics of the merging galaxies and their future trajectory.
