The galaxy presents a largely smooth morphology, appearing elliptical in shape, with a high degree of roundness. Its central region exhibits a bright, concentrated luminosity, suggesting a dense stellar population, possibly an older population. The galaxy displays a color gradient, transitioning from a yellowish-white core to slightly bluer, fainter edges. No distinct spiral arm structures are observed, nor is there evidence of a prominent disk. There are hints of minor disturbances or asymmetries in the outer regions. Overall, it appears to be a well-defined, relatively undisturbed system.
