The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The overall color gradient suggests an older stellar population, with a yellowish-orange hue concentrated towards the core, possibly indicating a higher density of evolved stars. The outer regions exhibit a bluer tint, hinting at the presence of younger, hotter stars, though their contribution appears minimal. There is a subtle suggestion of a disk-like component, but it is not prominently defined. The galaxy does not exhibit any clear signs of ongoing mergers or major disturbances in its morphology. Overall, this galaxy appears to be a relatively quiescent system, with a mass around 10^10 solar masses and a low star formation rate.
