The galaxy appears as a generally smooth object with a centrally concentrated bulge. It exhibits a spheroidal morphology, showing a high degree of circularity. There is a slight color gradient observed, with a bluer hue in the central region potentially indicative of ongoing star formation, and a shift towards redder colors in the outer regions. No clear spiral arms or disk features are discernible, though the central bulge is very bright. The galaxy doesn't appear to be undergoing any major mergers or disturbances.
