The galaxy presents as a largely featureless elliptical structure. Its morphology is predominantly smooth, with a high degree of central concentration. The isophotes appear generally round, with only a slight deviation toward an elongated shape. The galaxy exhibits a color gradient, trending from a yellow-white core to a reddish outer halo. The central region is bright, suggesting a substantial population of older stars. There is no evidence of ongoing major merger activity, although subtle asymmetries in the outer regions cannot be ruled out. The overall appearance suggests a relatively evolved galaxy with a low star formation rate.
