The galaxy presents as a moderately bright, elliptical-shaped object with a smooth, diffuse appearance. Its core exhibits a high concentration of light, which diminishes gradually towards the outer regions. There is little evidence of spiral arms or other distinct morphological features. The color gradient indicates an older stellar population, with a yellowish hue concentrated in the central bulge. Minimal dust lanes or star-forming regions are apparent, consistent with a low star formation rate. The galaxy appears relatively undisturbed, showing no signs of major mergers or tidal interactions.
