The galaxy presents as a relatively smooth, elliptical-like structure. There is a prominent central bulge that appears roughly spherical and displays a yellowish-orange hue, indicating an older stellar population with minimal ongoing star formation. The light diminishes gradually from the center outwards, suggesting a lack of distinct spiral arms or other prominent features. A subtle bluish tint surrounds the yellowish core, potentially indicative of a younger, hotter stellar population, although the effect is minimal. Overall, the galaxy appears relaxed and undisturbed, without evidence of recent mergers or tidal interactions. Its shape suggests an evolved system, likely with a substantial mass concentrated in the bulge.
