The galaxy appears to be in the late stages of a major merger. It presents as a luminous, elliptical-like structure with a prominent, bright core region and a slight green-yellow hue. Evident are two distinct, concentrated nuclei within the core, separated by a small distance, suggesting the ongoing coalescence of two separate galaxies. The system is centrally concentrated, with a relatively smooth overall appearance, hinting at an advanced stage in the merging process. The faint, extended light surrounding the merging nuclei may be tidal debris resulting from the gravitational interaction and disruption of the progenitor galaxies. The overall morphology leans toward a spheroid shape, suggesting a system that is increasingly dominated by random stellar motions.
