The galaxy presents as a single, relatively smooth, and concentrated light source. The central region displays a bright, yellowish hue, suggesting a high concentration of older stars. Moving outwards from the core, the light gradually decreases in intensity. The galaxy appears largely spheroidal, with no apparent spiral arm structures or a significant disk component. There is a faint, diffuse halo surrounding the central bulge, displaying subtle blue-ish tints. The overall structure indicates that this galaxy is likely an elliptical galaxy, with little ongoing star formation. Faint features may indicate a minor disturbance.
