The galaxy presents a smooth, elliptical morphology. The core exhibits a concentrated, bright yellow-orange hue, indicative of an older stellar population. Fainter greenish emission is observed in the galactic outskirts, potentially suggestive of ongoing, albeit subdued, star formation. The overall structure appears relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions. The galaxy exhibits an elongated shape, deviating from a perfect sphere. No distinct spiral arms or bar structures are discernible from the observation.
