The galaxy presents a largely smooth, elliptical morphology. The light is concentrated towards the center, indicative of a prominent galactic nucleus. The galaxy appears relatively undisturbed, exhibiting no signs of major merging events or tidal tails. There is a subtle color gradient, transitioning from a yellow-white hue in the core to a slightly redder tone in the outer regions, suggesting an older stellar population is more common in the galaxy's halo. The overall rounded shape and the lack of distinct spiral arms or a defined disk further support its classification as an elliptical galaxy.
