The galaxy presents as a system undergoing an interaction or possible merger. The primary body exhibits a generally smooth morphology, with a slightly elongated, though largely amorphous, structure. There is some evidence of possible tidal tails or disrupted structures extending from the main body, although the image resolution makes definitive identification difficult. Color gradients suggest differential stellar populations, with a central region exhibiting a yellowish-white hue indicative of older stellar populations, and bluer tints evident in the surrounding regions, potentially indicating ongoing or recent star formation. The light from the galaxy indicates it may be relatively massive, suggesting a potential elliptical classification. The secondary body displays a more irregular and concentrated core. Overall, the system appears to be dynamically active with ongoing gravitational disturbances.
