The galaxy presents as a singular, relatively smooth, and concentrated object. The morphology appears elliptical, with no visually discernible spiral arms or bar structures. The light distribution suggests a concentrated central bulge that fades gradually outwards. The galaxy displays a color gradient, transitioning from a reddish hue at the core to a bluer tint in the outer regions. This may indicate older stellar populations are centrally concentrated, while younger stars exist at the edges. There are no obvious signs of tidal disturbances or major mergers. It appears to be a relatively undisturbed system. The galaxy is well-defined, indicating that it is either close or particularly bright.
