The galaxy presents a largely smooth and elliptical morphology. The light is concentrated towards the center, indicating a prominent bulge. The galaxy appears to have a high degree of rotational symmetry. There are no obvious spiral arms or significant dust lanes visible. The color gradient transitions from a yellowish-white core to a dimmer reddish halo, suggesting an older stellar population. The overall structure points towards a galaxy which has undergone substantial spheroid formation. There appears to be no ongoing major merger or tidal disruption event. It seems to be a relatively undisturbed system.
