The galaxy presents a largely smooth and symmetrical morphology. It exhibits an elliptical shape, appearing moderately rounded rather than elongated. The central region is characterized by a bright, concentrated core, indicating a high density of stars and potentially the presence of a supermassive black hole. The galaxy displays a color gradient, transitioning from a yellowish-white hue in the core to a more reddish-orange tint in the outer regions. This color distribution suggests an older stellar population dominates the outer parts of the galaxy with relatively little ongoing star formation. There is no prominent disk structure or spiral arms, which further supports its classification as an elliptical galaxy. Additionally, there are no obvious signs of recent or ongoing mergers or tidal disturbances. The galaxy appears relatively undisturbed and isolated within the observed field.
