The galaxy presents as a generally smooth, elliptical morphology. The core exhibits a high degree of concentration, appearing bright and yellowish-white, which suggests a concentration of older stars. The light gradually diminishes outwards from the core, with the outer regions appearing more reddish, potentially indicating an older stellar population and/or dust absorption. There are no readily apparent spiral arms or distinct features, giving it a largely featureless appearance. The galaxy's shape is slightly elongated. There is no evidence of any major ongoing merger activity or significant tidal disturbance.
