The galaxy presents as a generally smooth, elliptical morphology. The central region exhibits a high concentration of light, appearing yellowish-white, which likely indicates an older stellar population. The isophotes appear somewhat elliptical, but trending toward round. There is a subtle color gradient as one moves outwards from the center of the galaxy; the outer regions become progressively more red. There is a possibility of a minor disturbance in the lower right quadrant of the galaxy, evidenced by a faint elongation that is redder in color. Overall, the galaxy appears to be relatively undisturbed.
