The galaxy appears as a somewhat amorphous, relatively smooth structure with a concentration of light in what may be a central region. I tentatively observe a triple galaxy merger, with three distinct, luminous cores possibly representing the nuclei of the merging galaxies. These nuclei appear embedded within a common envelope of fainter, diffuse light. Given the smooth appearance and lack of strong spiral arm structures, and the observed red color index, this system likely consists of relatively evolved galaxies undergoing interaction. There are hints of minor tidal disturbances or asymmetries in the outer regions, supporting the merger hypothesis. Based on the estimated redshift, the galaxy is seen as it was at a younger stage of the Universe's evolution. Given the estimated mass and star formation rates, star formation appears to be quenched. The morphology of the galaxy would be classified as elliptical or irregular. 
