The galaxy presents a largely smooth, elliptical morphology. Its color is predominantly yellow/orange, suggesting a relatively older stellar population with a lesser contribution from recent star formation. There are faint hints of slightly bluer light in the outer regions, hinting at a possibility of some younger stars being present within its galactic halo. The galaxy appears well-defined and centralized with no apparent signs of tidal disruption or major merger events. The roundness of the galaxy indicates a relatively low angular momentum or that it is being viewed along its primary axis. There is a possible hint of a minor interaction or disturbance.