The galaxy presents an elongated, elliptical morphology. The light distribution appears relatively smooth and centrally concentrated, with a gradual decrease in intensity moving outward from the core. The central region exhibits a yellowish-white hue, potentially indicating a population of older stars. There is a subtle color gradient, with the outer regions appearing slightly bluer, which could imply a younger stellar population within a disk component. No prominent dust lanes or spiral arm structures are discernible in the image. Overall, the galaxy appears relatively undisturbed, exhibiting characteristics consistent with an elliptical galaxy.
