The galaxy presents a primarily smooth morphology. It appears largely spheroidal, with an intermediate roundness. There is a dominant central bulge of higher luminosity. The outer regions exhibit a less concentrated, diffuse halo extending beyond the central region. There is no apparent spiral arm structure or strong bar feature. No obvious signs of active galactic nuclei or strong star formation are apparent in this image, though there are some indications of recent merging activity in the form of faint tidal tails.
