The galaxy presents as a centrally concentrated object with a relatively smooth and featureless overall appearance. The morphology appears predominantly elliptical or lenticular due to the lack of discernible spiral arm structures. The light distribution is centrally concentrated, with a gradual decline in surface brightness outwards from the core. The core region exhibits a yellowish-white hue, possibly indicative of an older stellar population, while the outer regions appear slightly redder. There are no obvious signs of recent major merger events, such as tidal tails or shells. The galaxy exhibits a relatively compact size with little to no visual disturbance.
