The galaxy presents a smooth, elongated morphology, suggesting a classification as an elliptical galaxy. The light distribution appears concentrated towards the center, with a gradual decrease in intensity towards the edges. The observed color is slightly redder, indicative of an older stellar population and reduced star formation activity. There is no evidence of spiral arms or a prominent disk structure. The overall appearance suggests a relatively undisturbed system, showing no strong signs of ongoing mergers or significant tidal interactions.
