The galaxy presents as a relatively smooth, elliptical structure. The central region exhibits a high concentration of luminosity, appearing a yellowish-white hue. Moving outward from the center, there is a gradual decrease in surface brightness. There appears to be a subtle color gradient, transitioning from the yellowish core to a slightly bluer, green tinged periphery. This suggests a possible difference in stellar populations between the central bulge and the outer regions. There is no clear evidence of spiral arms, bars, or significant dust lanes. The overall morphology indicates a evolved system, potentially with ongoing, but relatively low levels of star formation. The smooth appearance indicates that it is unlikely that it is currently undergoing a major merger.
