The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a moderate degree of roundness. The central bulge is prominent and displays a yellowish-white color, suggestive of an older stellar population. The outer regions of the galaxy show a gradual decrease in brightness, with subtle hints of bluer hues, possibly indicating regions of younger stars or ongoing, though limited, star formation. There is no clear indication of a distinct disk structure or spiral arms. Overall, the galaxy’s morphology appears relatively undisturbed, showing no signs of major mergers or significant tidal interactions. The light distribution suggests a system dominated by an evolved stellar population, consistent with a low star formation rate.
