The galaxy presents an overall elliptical morphology. The central region displays a high surface brightness, appearing concentrated and nearly spherical in shape. This core exhibits a yellowish-white color, suggestive of an older stellar population. Moving outward from the core, the galaxy gradually fades in intensity. There is some indication of a subtle disk feature, but this is not very clear, and might simply be a slight difference in color within the outskirts of the galaxy. No distinct spiral arms or prominent dust lanes are visible. The outer regions are more diffuse and display a slightly bluer color, which may be due to the presence of younger stars, though the amount of recent star formation appears very low. There is no apparent sign of any major interactions or mergers and the overall structure appears relatively undisturbed. The galaxy appears very round and undisturbed.
