The galaxy appears to be a merging system comprised of at least two distinct components. One component exhibits a smoother morphology, likely an elliptical galaxy, characterized by a centrally concentrated luminosity profile and a yellowish-white hue. The other component displays a more irregular structure with a distinct orange coloration. The two components are in close proximity, showing signs of tidal interaction and potential gravitational distortion. There is no clear spiral arm structure evident in either component. The system exhibits an overall moderate luminosity, as expected at its relatively high redshift. A minor disturbance or merging event is in progress as indicated by the irregular morphology and signs of interaction.
