The galaxy presents as a relatively compact, elliptical object with a smooth, diffuse light distribution. Its color profile indicates a dominant population of older stars, evidenced by the yellowish-orange hue, suggesting low levels of current star formation. There is no discernible structure, such as spiral arms or a prominent galactic bar. The galaxy appears largely undisturbed, showing no strong signs of tidal interactions or ongoing mergers. It possesses a spheroidal shape.
