The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears largely featureless. Faint extensions are visible which may indicate a more disk-like structure that is observed edge on. There is a slight gradient in color, becoming bluer toward its faint extremities and redder toward the central core, potentially indicating differing stellar populations or dust distribution. Overall, the galaxy appears to be relatively undisturbed and does not show obvious signs of ongoing major mergers, although there may be minor disturbances.
