The galaxy presents as a relatively smooth, elliptical structure. Its overall shape is close to being round, with a slight elongation giving it an intermediate appearance between a perfect circle and an elongated ellipse. The color profile suggests an older stellar population dominating the central regions, indicated by the yellowish-red hue. There is some evidence of bluer, potentially younger stars distributed throughout the galaxy, particularly in the outer regions, which could indicate ongoing, though low levels of star formation. There are no readily discernible spiral arms or bar structures; it is primarily characterized by its smooth morphology and relatively homogenous distribution of light, with a slight concentration towards the center. There are no indications of major mergers or significant tidal disturbances, suggesting a relatively quiescent evolutionary history.
