The galaxy presents a smooth, elliptical morphology. Its overall color profile appears slightly redder in the central regions, suggesting an older stellar population concentrated towards the core. The outer regions exhibit a gradual decline in surface brightness, with a less defined edge. No distinct spiral arms or dust lanes are discernible. The galaxy appears relatively undisturbed, with no signs of major mergers or tidal interactions. The overall shape is somewhat elongated, implying a non-zero ellipticity.
