The galaxy appears to be an elliptical galaxy with a smooth, featureless morphology. It is elongated in shape, with the ratio of its major to minor axis being roughly 2:1. The central region of the galaxy is more luminous and exhibits a yellow-white hue, possibly indicative of an older stellar population. Moving outward from the center, the galaxy's light gradually fades and transitions to a more blue-green tint, perhaps signifying younger stars or recent star formation in the outer regions. There is no discernible evidence of spiral arms or a prominent disk structure. No apparent merging signatures or tidal disturbances are visible, suggesting a relatively undisturbed evolutionary history.
