The galaxy presents as a centrally concentrated system with a smooth, elliptical-like morphology. The light profile exhibits a gradual decrease in intensity from the core outwards. A subtle colour gradient is observable, with the central region appearing more yellowish-white, potentially indicating an older stellar population or dust obscuration, while the outer regions show a slightly bluer hue, suggestive of younger stars. The overall structure lacks any prominent spiral arms or bar features. There is no evidence of a major ongoing merger, though very subtle disturbances cannot be ruled out. The galaxy appears relatively isolated.
