The galaxy appears as a merging system, exhibiting distinct features indicative of gravitational interaction. One component presents as a relatively smooth, rounded structure, displaying a whitish-green hue, potentially suggesting ongoing star formation. The second component is more elongated, with an orange color, perhaps indicating an older stellar population or dust obscuration. Significant tidal disruption is apparent, with morphological disturbances evident, including bridges of material stretching between the two primary structures. This suggests a late-stage merging event, where the galaxies are in close proximity, heavily influencing each other's structure.
