The galaxy presents as an elliptical or lenticular type. The light profile appears relatively smooth and centrally concentrated, lacking prominent spiral arms or a distinct disk-like structure, though it may possess a weak disk component. There appears to be a color gradient, transitioning from a yellow-white core to a slightly bluer halo or outer region. This may indicate a difference in stellar populations, with older stars dominating the core and younger stars possibly contributing to the outer regions. The galaxy appears relatively undisturbed, showing no strong signs of recent major mergers or tidal interactions, though there may be slight asymmetry in the halo that could possibly be due to a minor merger. The apparent size is small.
