The galaxy presents as a relatively smooth elliptical system. Its overall shape is elongated, appearing as a flattened spheroid. The core region displays a bright, concentrated luminosity that gradually fades towards the outer edges. There is little indication of spiral arms or significant dust lanes. Faint color variations are visible, transitioning from a central yellowish-white hue to a bluish-white tint in the extended halo. The observed morphological features suggest that star formation activity is low. There is no obvious disruption or tidal feature to suggest it is merging. The image is consistent with an elliptical galaxy with an effective radius of approximately 3 kpc.
