The galaxy presents as a smooth, elliptical-like object with a concentrated central bulge that fades out into the surrounding space. The core exhibits a bright, yellowish hue, suggesting a population of older stars. The overall shape is somewhat rounded, with minimal apparent structural features such as spiral arms or bars. The outer regions appear less defined and more diffuse, transitioning subtly into the background sky. There are no obvious signs of ongoing mergers or major tidal disturbances. The galaxy's color profile implies a relatively low rate of star formation, consistent with a more evolved stellar population.
