The galaxy presents as a generally smooth, centrally concentrated object with an elliptical morphology. The central bulge region appears bright and relatively featureless. There is subtle color variation across the galaxy, trending towards slightly bluer hues in a faint, extended region, possibly indicative of recent star formation. There is no clear evidence of spiral arm structure or a prominent dust lane, which would support its classification as an elliptical galaxy. It exhibits no signs of major disturbance, although subtle asymmetries exist that may suggest minor interactions or past merger events. The overall structure appears fairly rounded.
