The object presents as a merging system or a single galaxy with significant tidal disruption. The morphology suggests a late-stage merger with two distinct but overlapping central concentrations of light, potentially indicating the cores of the progenitor galaxies. The overall color is yellowish-red, implying an older stellar population with less ongoing star formation. The system appears relatively compact, although there are faint extensions of light, hinting at tidal tails or disrupted stellar material. Based on the color, the object likely contains a considerable amount of older stars. The internal structures are not well-defined, likely due to the ongoing interaction.
