The observed galaxy presents a complex morphology, suggestive of an ongoing or recent interaction. There appears to be two primary luminous regions or cores, indicating at least two distinct galactic components. The larger component is more luminous with a yellow/orange center, and a bluish outer region. The smaller core appears similar. There is visible distortion and asymmetric tidal features extending outwards, likely due to gravitational interactions. The overall color profile suggests a mix of older stellar populations in the central regions and younger, bluer populations within the disk-like structures. The galaxy has a perturbed structure, exhibiting characteristics of a merging system.
