The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a predominantly elliptical morphology, showing a high degree of circularity. The galaxy's light profile suggests a lack of prominent spiral arm structures or a distinct disk component. There is a subtle colour gradient, with the central region displaying a slightly redder hue, possibly indicating an older stellar population or increased dust extinction, surrounded by a fainter and slightly bluer halo, potentially indicating younger stars. There are no clear signs of major mergers or tidal disturbances within the visible structure. The absence of significant features suggests this galaxy is likely an evolved system.
