The galaxy presents as a relatively smooth and centrally concentrated object, indicative of an elliptical morphology. The core is bright and yellowish, suggesting a population of older stars. The outer regions exhibit a gradual decline in surface brightness, and are slightly more spherical in shape. There is a slight asymmetry or subtle disturbance visible, implying a potential past interaction or minor merger. Star formation appears to be low throughout. Overall, the galaxy appears to be a relatively evolved system.
