The galaxy presents a generally smooth and elliptical morphology. The central bulge appears concentrated and exhibits a yellowish-orange hue, indicative of an older stellar population. Moving outward from the core, the galaxy's luminosity gradually decreases, transitioning to a fainter, bluish halo. There is a subtle suggestion of a disk-like structure, although the smoothness of the overall profile suggests it is not the dominant feature. No significant tidal tails or indications of recent major merger events are immediately apparent. Minor disturbances cannot be ruled out, but the galaxy appears relatively relaxed and well-defined. There is no dust that is readily apparent in the image.
