The galaxy appears to be in a system of two interacting galaxies. The larger of the two galaxies exhibits a smooth morphology, with a slightly elliptical shape. The color profile appears to be somewhat redder, suggesting an older stellar population and a suppression of star formation. 

The smaller galaxy displays a less defined structure and a marginally bluer hue. This suggests a younger stellar population or ongoing star formation. The overall structure is more diffuse and the colors appear less concentrated in the center. The two galaxies appear to be in a close interaction or merger phase, causing some tidal disruption in both galaxies.
