The galaxy presents as a relatively smooth, centrally concentrated object with a near-circular morphology. Its color gradient transitions from a yellow-orange core to a slightly bluer halo, implying a potential variation in stellar population ages and compositions. The galaxy exhibits no obvious spiral arm structures or significant dust lane features. There is very little evidence of any tidal disturbances or merging activity. This galaxy may be an elliptical galaxy, based on its smooth profile and lack of disk features.
