The galaxy presents a generally smooth and concentrated morphology. The central region exhibits a bright, yellowish-white core, suggesting an older stellar population. The galaxy's light gradually decreases in intensity from the core outwards. The overall shape appears close to circular, lacking any distinct spiral arm features or bar structures. There are no obvious signs of major disturbances or ongoing merger activity, though minor asymmetries can't be ruled out due to the resolution. Overall, it is an elliptical galaxy that is relatively massive, with a low rate of star formation.
