The galaxy presents a smooth, elliptical morphology. The central region exhibits a bright, concentrated core. The overall color is yellowish-orange, suggesting a dominant population of older stars and a low rate of current star formation. The isophotes appear generally round. There is no discernible evidence of spiral arms, a bar, or ongoing major merger activity. Faint, subtle structures might be present in the outer regions upon closer inspection, perhaps indicating minor tidal disturbances.
