The galaxy appears to be a relatively smooth, elliptical galaxy with a bright central core. It exhibits a spheroidal morphology, lacking any discernible spiral arms or a prominent disk structure. The light distribution suggests a high degree of central concentration, fading gradually outwards. Its color is predominantly a pale blue-white, hinting at a population of relatively young, hot stars although this color could be skewed by the redshift. There is no strong evidence of recent major merger activity or significant tidal disturbances in its immediate environment.
