The galaxy presents a smooth, elliptical morphology, lacking any discernible spiral arm structure. Its light profile appears centrally concentrated, with a gradual decrease in surface brightness towards the outer regions. The shape is moderately elongated, neither perfectly spherical nor highly flattened. There are no obvious signs of ongoing major mergers or significant tidal disturbances. Faint color gradients might be present, with a slightly bluer hue towards the central regions, suggesting the presence of a younger stellar population there compared to the redder outer halo. Overall, it is a relatively undisturbed, evolved system with intermediate mass. Star formation is present, but at a relatively low level.
