The galaxy presents an elliptical morphology, appearing largely smooth and featureless. It exhibits a pronounced central bulge that transitions into a more diffuse, extended halo. The color gradient indicates a higher concentration of older stellar populations in the bulge, exhibiting a yellowish-orange hue, while the outer regions appear slightly bluer, possibly indicating the presence of younger stars or ongoing star formation, albeit at a relatively low rate. There are no clear signs of spiral arms or significant dust lanes. The overall shape is somewhat elongated, suggesting a possible deviation from a perfectly spherical structure. The image doesn't show any signs of recent or ongoing major mergers or interactions with other galaxies, with no prominent tidal tails or other disruptive features visible.
