This galaxy presents as a relatively smooth, centrally concentrated object. The light profile appears to be concentrated in the center, which graduates into a more diffuse halo surrounding the core. The light emanating from the galaxy appears to be concentrated toward the redder portion of the spectrum, indicating a greater population of older stars. There is a small hint of green, which could mean some star formation is occurring, however, there isn't any well-defined spiral structure or dust lanes visible. Overall, the galaxy appears to be elliptical or lenticular in nature.
