The galaxy presents as a relatively smooth, elliptical morphology. The light distribution appears concentrated towards the center, with a gradual decrease in intensity outwards. There is no discernible spiral arm structure or distinct features indicative of recent major merger events. The galaxy exhibits a slight elongation, deviating marginally from a perfectly circular shape, with the major axis oriented roughly horizontally in the image. The color profile appears relatively uniform across the galaxy, although the central regions may have slightly redder hues, which could be due to older stellar populations. Overall, the galaxy seems consistent with an early-type galaxy that has undergone significant evolution and stabilization.
