The galaxy presents as a relatively smooth, lenticular-like structure. The overall color appears yellowish-white, suggesting a population of older stars. The light is centrally concentrated with an apparent bulge. There is a hint of a disk-like component extending outwards from the central bulge, but no spiral arms or distinct features are observed. The object is elongated along one axis, appearing cigar-shaped rather than perfectly circular. There are no obvious signs of active galactic nuclei activity, or tidal disturbance to suggest recent merger events. Star formation appears to be suppressed, as indicated by the lack of blue light associated with younger stars. The absence of strong features suggests that the galaxy is a relatively quiescent system, past its peak period of star formation.
