The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a fairly round morphology, with a slight deviation from perfect circularity. The central region displays a yellowish-white hue, suggesting an older stellar population and less active star formation in the core. Moving outward from the core, the color shifts towards a bluer tone, indicating the presence of younger, hotter stars. There is a subtle indication of a disk, though the structure is not sharply defined. There is no strong evidence of ongoing major mergers or significant tidal disturbances, although a slight asymmetry might suggest minor past interactions. Overall, the galaxy appears to be a relatively evolved system, possibly transitioning towards a more quiescent state.
