The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge region that gradually fades into a less dense outer halo. The color gradient transitions from a yellowish-white core to a more reddish-tinged periphery. There are no readily apparent spiral arm structures or significant dust lanes visible. The morphology suggests a lack of recent major merger events, with only minor asymmetries or disturbances present. The galaxy appears to be relatively isolated in the field.
