The galaxy appears as a centrally concentrated object with a generally smooth morphology. The light distribution suggests an elliptical or lenticular galaxy type, lacking prominent spiral arm structures. It exhibits a relatively high degree of rotational symmetry and circularity. There may be a subtle asymmetry or minor tidal disturbance present, potentially indicative of a past or ongoing interaction. Overall color indices suggest a population of older stars and a very low rate of star formation. The approximate physical size is relatively small, with a estimated mass slightly over 10^10 solar masses.
