The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated, bright yellowish-white luminosity, suggesting an older stellar population. The light profile gradually diminishes from the core outwards, showing no prominent spiral arms or distinct features. The shape appears largely rounded, with a slight deviation towards an intermediate ellipticity rather than a perfectly circular form. There is no visual evidence of any major merging events or significant tidal disturbances. Faint blue light on the outskirts suggests the possibility of some young star formation on the edges of the galaxy. The system appears relatively undisturbed and isolated.
