The galaxy presents as a smooth, elliptical structure. It has a concentrated central bulge that appears largely featureless. The color gradient suggests a higher concentration of older stellar populations in the core, which shifts to a slightly bluer hue towards the outer regions of the galaxy. The overall morphology is elongated with a high degree of roundness, but not perfectly spherical, appearing to be somewhere in between. There are no obvious signs of spiral arms, bar structures, or ongoing major merger activity. Minor disturbances might be present, though they are subtle. The galaxy's apparent smoothness indicates it may have undergone significant dynamical relaxation.