The galaxy appears as an elliptical or lenticular system, exhibiting a smooth, concentrated light distribution with no distinct spiral arms or bar structures visible. The galaxy displays a yellowish-white hue, which suggests a population of older stars. The galaxy exhibits a moderate degree of roundness, appearing somewhat flattened but not highly elongated. The overall structure indicates a relatively evolved system, likely with a significant spheroidal component and a reduced rate of star formation. There is no indication of any major mergers or tidal disturbances.
