The galaxy appears as a centrally concentrated, elliptical-like structure. The core exhibits a bright, yellowish hue, suggesting an older stellar population and potentially lower rates of recent star formation. A faint, greenish-blue halo surrounds the central region, possibly indicative of some ongoing, though subdued, star formation or ionization processes. The overall form appears relatively smooth and undisturbed, showing no clear signs of major mergers or significant tidal distortions. The general roundness of the galaxy is notable, with only very minor deviations from a perfectly circular morphology.
