The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology with a roughly round shape. The color profile indicates a pronounced central bulge, appearing more yellow-orange, which suggests an older stellar population dominating the core. Moving outwards from the center, the galaxy's color shifts to a slightly bluer hue, potentially indicative of more recent star formation activity in the outer regions, though this is not strongly evident. No distinct spiral arms or bar structures are visible. There is a slight indication of possible minor disturbances in the outer disk. Overall, the galaxy appears to be a relatively undisturbed, mature system.
