The galaxy presents as a centrally concentrated, elliptical-like structure. It exhibits a smooth, diffuse light profile, with the brightest region located at its core. There is a color gradient visible, transitioning from a yellowish-white center to a slightly redder hue in the outer regions, suggesting an older stellar population predominating, particularly in the outskirts. The shape is approximately rounded, with only slight deviations from a perfect circle, indicating minimal recent merger activity or significant tidal disturbances. No prominent spiral arms or distinct dust lanes are discernible in this image. Overall, the galaxy appears to be a relatively undisturbed, evolved system.
