The galaxy presents an overall elliptical morphology, appearing predominantly smooth in structure. The central region exhibits a concentrated luminosity, displaying a yellow-white hue. Moving outwards from the core, the color shifts towards a more diffuse, yellowish tone, which implies a less concentrated stellar population in the outer regions. There is a slight hint of a disk like feature to the galaxy. There are some faint blue tinges in the outer parts, suggestive of some areas of possible star formation. There is no apparent evidence of strong spiral arm structures or a prominent bar. There is no obvious indication of major mergers or tidal disturbances, but there could be some minor gravitational disturbances due to the slight asymmetrical features of the galaxy.
