The galaxy presents a generally smooth morphology. It exhibits a concentrated, spheroidal shape with a bright, luminous core. The light distribution decreases steadily from the center outward. There is little discernible structure such as spiral arms or a prominent disk. The galaxy appears relatively isolated, with no obvious signs of recent major mergers or tidal disturbances. The color profile suggests an older stellar population, with a redder hue becoming dominant toward the outskirts.
