The galaxy presents as a centrally concentrated object with a smooth, largely featureless appearance, with the absence of prominent spiral arms or a well-defined disk structure. Its overall shape is approximately elliptical, though it exhibits a slight deviation from perfect roundness. The color profile indicates a relatively evolved stellar population. The central region appears brighter and more yellow. There are no obvious signs of recent major merger events, although subtle irregularities might hint at minor disturbances. Based on its red shift, it is at a considerable distance from the observer. The object’s mass is estimated to be quite high, yet it exhibits very little to no ongoing star formation activity.
