This galaxy appears to be in the process of a significant interaction, potentially a major merger. Its morphology is disturbed, exhibiting an irregular shape. Two distinct, bright cores are visible, suggesting the nuclei of the merging galaxies. A diffuse halo of light surrounds the central region, possibly indicative of tidal debris and scattered starlight resulting from the gravitational interaction. Some faint extensions or tails are hinted at, though the low resolution makes them difficult to definitively characterize. The color profile shows a mix of bluer hues in the central regions and more reddish tones in the outer regions, possibly indicating differing stellar populations or dust distribution across the system. Given the apparent disturbance and merging activity, further spectroscopic and high-resolution imaging would be beneficial for a complete understanding.
