The galaxy presents as a relatively smooth, elliptical structure, with a concentrated central bulge that is brighter and more intensely colored. There is a slight elongation to the shape, suggesting it may not be perfectly spherical. The galaxy exhibits a color gradient, transitioning from the yellow/orange hue of the core to a more subdued, slightly bluer tone in the outer regions. This color distribution might indicate older stellar populations concentrated centrally and hints of ongoing, though subdued, star formation in the outskirts. No distinct spiral arm structures or significant dust lanes are discernible, supporting the classification of a more evolved system with minimal ongoing major star formation episodes. There are no visible signs of a major ongoing merger event.
