The galaxy presents as a smooth, luminous object, exhibiting an elliptical morphology. There is indication of a possible merger event. The galaxy's light profile appears centrally concentrated with a gradual decrease in intensity outwards. There is a slight disturbance in the light profile of the object. Overall, the galaxy seems to be in a late stage of its evolution, indicated by its smooth appearance. Further investigation with higher resolution imaging is required to ascertain the nature of the disturbance to the light profile.
