The galaxy appears to be a relatively smooth, elliptical-like structure. The central bulge exhibits a yellowish hue, suggesting an older stellar population. Moving outward from the core, the color profile shifts towards a slightly bluer tone, hinting at the presence of some younger stars or ongoing, though perhaps limited, star formation in the outer regions. No distinct spiral arms are discernible. There is a faint suggestion of a disk-like component, however it is unclear if that is an artifact of the bulge. The overall morphology suggests a system that is largely settled with minimal signs of active mergers or major disturbances. The light is heavily concentrated towards the center, fading gradually towards the edges. It is approximately symmetrical.
