The galaxy appears as a centrally concentrated, elliptical-like system. It exhibits a smooth, largely featureless morphology, with a high degree of central light concentration. The galaxy displays a roughly spherical shape, with no obvious disk-like structures or spiral arms visible in this image. The light profile suggests a gradual decline in brightness moving outward from the core. Its color profile implies a relatively homogenous stellar population, with an overall yellowish-orange hue suggesting evolved stars dominating its composition. There are no apparent signs of ongoing major mergers or significant tidal disturbances in this image, indicating the system is relatively relaxed and isolated.
