The galaxy presents a predominantly smooth, elliptical morphology. Its light profile appears centrally concentrated, with a gradual decrease in intensity towards the outer regions. The core exhibits a yellowish hue, suggesting a population of older, evolved stars. Surrounding the central region, a subtle blueish tint can be observed, potentially indicative of a younger stellar population or ongoing, albeit subdued, star formation activity. The overall shape is moderately elongated, but lacks distinct features such as spiral arms or a prominent disk. The absence of significant irregularities or tidal tails suggests that the galaxy is relatively undisturbed, with no recent major merger events apparent.
