The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The core region displays a pronounced luminosity, decreasing radially outwards. A slight color gradient is discernible, with the central region appearing more yellow-white, possibly indicating an older stellar population. Fainter, bluer regions are distributed within the outer halo. There appears to be no spiral structure, bar, or significant dust lane visible in the image. The overall structure suggests a mature galaxy which does not appear to be undergoing major active star formation.
