The galaxy presents as a moderately luminous, early-type system, with a spheroid-dominant morphology. The overall light distribution is smooth and centrally concentrated, exhibiting a high degree of rotational symmetry. The galaxy appears elliptical, with a suggestion of slight elongation, but is generally round. There is no apparent spiral structure. The color is generally red-shifted and homogenous across the visible light spectrum and it does not seem to have any major disturbances or mergers occurring. There are no distinct features such as prominent dust lanes or tidal tails. Overall, the galaxy appears to be relatively evolved, consistent with a passively evolving stellar population and a low star formation rate.
