The galaxy presents a complex morphological structure, appearing to be undergoing a significant interaction or merger. Two distinct, relatively bright, spheroidal components are observed. The brighter, more yellow component lies above and is more diffuse, while the bottom spheroidal component appears slightly more compact with hints of blue. There is a tidal tail connecting the two galaxies and there appears to be some interaction going on between the two. 

The overall color profile suggests an older stellar population dominating the galaxy, with evidence of ongoing or recent star formation within the less bright galaxy, suggested by the blue color. Given the redshift, the galaxy is significantly luminous.
