The galaxy presents as a somewhat smooth, centrally concentrated object, with a slightly elliptical morphology. There's a hint of a disk-like structure, though the smoothness suggests a dominant spheroidal component. The galaxy appears yellowish-white, indicative of an older stellar population. There's a possible minor disturbance, or perhaps a tidal feature, on one side. A small percentage of the galaxy might be composed of actively merging components. The galaxy displays a high mass, with an intermediate star formation rate.
