The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a high concentration of light, appearing a pale yellow-white, indicating a dominant population of older stars. The light intensity decreases gradually from the core outwards, with no distinct spiral arm structures or prominent dust lanes visible. The outer regions show a faint, diffuse halo with a slight blueish color, possibly indicating recent star formation or a younger stellar population compared to the core. The shape is predominantly round, with no obvious tidal features or major disturbances suggesting recent major merger activity, although there may be some minor irregularity in the outermost reaches of the halo. Overall, the galaxy appears as a well-formed, evolved system with ongoing, but subdued, star formation.
