This galaxy appears to be a relatively smooth, elliptical galaxy with a high degree of central concentration. The morphology suggests a classification leaning toward an early-type galaxy. The object exhibits a roughly spherical shape, with a noticeable lack of defined spiral arms or a prominent disk structure. The color gradient transitions from a yellowish core to a slightly redder halo, indicative of an aging stellar population and potentially lower levels of on-going star formation within the galactic body. There is no visible evidence of any major mergers or significant tidal disturbances affecting its overall form, suggesting it has been relatively undisturbed for a significant period. The galaxy displays a smooth, symmetric light profile, likely due to the evolved nature of its stars and the lack of significant dust obscuration.
