The galaxy presents as a centrally concentrated, elliptical-like system with a smooth, diffuse appearance. It displays a radial color gradient, transitioning from a yellow-white core to a slightly redder halo. There is no apparent spiral arm structure or significant dust lane obscuration visible. The overall morphology suggests a relatively evolved system, potentially an elliptical galaxy or a lenticular galaxy viewed face-on, lacking prominent star-forming regions. The galaxy appears relatively isolated, showing no obvious signs of tidal interactions or major mergers. The light distribution is fairly regular, indicating a dynamically relaxed state.
