The galaxy presents an elliptical morphology, exhibiting a smooth, featureless structure with a slight elongation. The color gradient transitions from a reddish-orange core to a greenish-blue outer region, suggesting potential variations in stellar populations or dust distribution across the galaxy. The overall shape is consistently smooth, with no readily apparent signs of tidal disturbances, major mergers, or distinct spiral arms. Subtle hints of a disk-like structure may be present, although the dominant characteristic is one of a spheroid. The galaxy appears relatively isolated.
