The galaxy presents as a generally smooth object with an elliptical morphology. It exhibits a concentrated central bulge region that gradually fades into an outer halo. The light distribution suggests a fairly uniform stellar population, with a dominant yellowish-red hue. There is no clear evidence of spiral arm structures or significant dust lanes. Minor disturbances may be present, but overall the object appears relatively undisturbed, showing no clear signs of a recent major merger event. The galaxy has a relatively high redshift, and is likely a very massive object with relatively low ongoing star formation.
