The galaxy presents a largely elliptical morphology, appearing mostly smooth and featureless. The central region exhibits a concentrated, bright core, suggestive of a significant stellar population density. A subtle color gradient can be observed, transitioning from a yellowish-white core to a slightly bluer halo, possibly indicating varying stellar ages or compositions with distance from the galactic center. There is a slight elongation of the galaxy's overall shape, however the galaxy is mostly round. Overall, the galaxy doesn't show signs of interactions or mergers.
