The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a high surface brightness, indicating a concentrated stellar population likely dominated by older, redder stars. Moving outward from the core, the light intensity decreases gradually, displaying a diffuse halo. A subtle color gradient is observed, transitioning from a yellowish-white core to slightly bluer hues in the outer regions, possibly suggesting some ongoing, but minimal, star formation at the galaxy's periphery. No distinct spiral arms or significant dust lanes are apparent, further supporting its classification as an elliptical galaxy. Some minor disturbances cannot be ruled out. The overall roundness suggests a relatively low inclination angle with respect to our line of sight.
