The galaxy appears as an elliptical, centrally concentrated system. The core exhibits a bright, reddish hue, which suggests an older stellar population. Moving outwards from the center, the light profile gradually fades, transitioning to a more greenish-yellow color. This could indicate the presence of younger stars or dust. The overall morphology suggests a relatively smooth structure with limited, subtle features. There are potential signs of very minor disturbances or tidal features in the outer regions of the galaxy, visible as faint extensions or asymmetries in the diffuse halo. The galaxy's shape is not perfectly spherical; it displays a slight elongation along one axis.
