The galaxy appears to be in the process of merging with another galaxy or experiencing a significant gravitational interaction. There are two distinct concentrations of light, suggesting two galactic cores. The primary concentration is more diffuse and shows a yellowish-white color, indicating an older stellar population. The secondary concentration appears more compact and redder, possibly indicating a later stage of star formation or dust obscuration. There is faint, greenish emission surrounding the primary concentration and connecting it with the secondary concentration which may suggest ongoing star formation in that region. Overall, the galaxy appears relatively smooth, suggesting a relatively evolved system, though disturbed by the ongoing interaction.
