The galaxy appears as a somewhat elongated, lenticular or early-type spiral system. Its overall color is predominantly yellowish-white, suggesting an older stellar population and a lower rate of ongoing star formation. There is a subtle hint of blueish light in the outer regions, indicative of some younger, hotter stars, although they are not dominant. The galaxy's light is centrally concentrated, with a smooth, diffuse profile, lacking prominent spiral arms or distinct features. It appears relatively undisturbed, exhibiting no signs of major mergers or strong tidal interactions. The galaxy displays intermediate roundness with only a very slight indication of a disk or other non-smooth features.
