The galaxy exhibits a morphology suggestive of an ongoing interaction or merger. Two distinct luminous regions are observed, indicating two galactic nuclei in close proximity. The larger of these regions exhibits a more diffuse, less concentrated appearance, while the smaller region appears more compact. There's evidence of tidal distortion and faint extensions that could represent tidal tails, although the image resolution limits definitive confirmation. The overall color profile suggests the presence of both younger, bluer stellar populations indicative of recent star formation and older, redder populations, particularly in the larger, more diffuse region. The system displays a moderate luminosity. The interacting system is roughly elliptical in overall shape. 
