The galaxy presents as a slightly elongated, lenticular-like structure with a relatively smooth appearance. Its color index suggests a mix of stellar populations, but appears more weighted toward older stars. The central bulge is subtly brighter than the disk, but lacks a highly concentrated nucleus. There is a slight indication of a disk structure. Possible minor disturbances present but no clear signs of major mergers or strong tidal features are observed. The galaxy appears to be relatively isolated, without obvious interacting companions within its immediate vicinity.
