The galaxy appears to be undergoing a significant merger event. The morphology suggests two distinct luminous components are interacting, possibly representing the cores of the merging galaxies.

There is evidence of tidal disruption, visible as faint, diffuse extensions surrounding the brighter central region. These features are asymmetric, with the brighter of the two components having a rounder shape and the second one being more oblong. 

Color gradients are present, with the core appearing yellower and the outer regions exhibiting bluer hues, indicating varying stellar populations and potentially active star formation in certain areas. The overall color index (G-Z) suggests a relatively evolved stellar population, but the merger could be triggering new star formation.
