The galaxy presents as a single, concentrated luminosity, appearing largely smooth and elliptical. The light distribution appears centrally concentrated, with a bright, yellowish core indicative of an older stellar population. The isophotes appear largely circular, suggesting minimal flattening. There is a slight color gradient, transitioning from a yellow center to a more green-shifted outer halo, which suggests the presence of some younger stars or ongoing, though limited, star formation in the outer regions. There is no discernible dust lane, spiral arm structure, or tidal features, which aligns with its classification as a relatively undisturbed elliptical galaxy.
