The galaxy presents as an elliptical morphology, with a smooth, diffuse light distribution. It exhibits a distinct central bulge that appears more concentrated and possesses a warmer color temperature, likely indicating an older stellar population. The outer regions of the galaxy are less defined and have a slightly cooler color temperature, showing a possible presence of younger stars. There appears to be a slight disk-like structure surrounding the central bulge. While there is no evidence of a major ongoing merger event, a minor asymmetry suggests a possible past interaction or minor disturbance. The overall color suggests an intermediate redshift.
