The object appears to be a galaxy undergoing a major merger. The morphology is disturbed, with a significant fraction of light concentrated in two distinct, relatively bright cores. The larger core exhibits a yellowish-white color, suggesting a population of older stars. The smaller core has a more reddish-orange hue, potentially indicating ongoing star formation and the presence of dust obscuration. There are faint tidal features or distortions visible, contributing to the overall irregular shape. The galaxy exhibits relatively smooth features between the cores, suggesting these may be galactic bulges beginning to coalesce.
