The galaxy presents as a largely featureless elliptical system. It exhibits a smooth, rounded morphology with a high degree of central concentration. The color profile suggests an older stellar population, with a dominant yellowish-orange hue in the core region, potentially indicating a greater abundance of evolved stars. There's a subtle color gradient towards the outer regions, trending slightly bluer. The galaxy's symmetrical shape implies a dynamically relaxed system, showing no prominent signs of recent or ongoing major mergers. The minor disturbances observed are negligible, with no signs of tidal tails, warps, or other strong gravitational interactions with nearby galaxies. The object's intermediate redshift indicates a considerable distance, suggesting it is being observed in a stage of its evolution further back in cosmic time. Star formation activity appears suppressed, consistent with the observed passive stellar population. 
