The galaxy presents as a centrally concentrated, elliptical-like structure. Its morphology is largely smooth, with a high degree of rotational symmetry. There is no apparent spiral arm structure or significant dust lane presence. The light distribution suggests a fairly uniform stellar population, though with a concentration of yellow to green colors in the center, indicating older stars. There is no visual evidence of recent major merger activity or significant tidal disturbances. It is a fairly compact galaxy. The overall color gradient transitions from yellow/green at the center to redder tones in the outer halo. There is minimal presence of blue light or color gradients in the outer portions of the halo suggesting a lack of active star formation.
