The galaxy appears as a moderately bright, elliptical-shaped object. It has a smooth, diffuse light distribution without any apparent spiral arms or distinct morphological features. The color gradient indicates a concentration of older stars toward the center, which emits a yellowish light, transitioning to a slightly bluer halo indicative of a small amount of younger stars. There is no evidence of a significant dust lane or tidal disruption. Faint red emissions appear, suggestive of minimal active star formation, likely in the outer regions. Overall, the galaxy exhibits characteristics consistent with a relatively evolved system with limited current star formation.
