The galaxy presents an elliptical morphology, appearing largely smooth and spheroidal in structure. It exhibits a concentrated central bulge which emanates light most intensely within the orange-red wavelengths. The overall color suggests an older stellar population within the main body of the galaxy. There is a slight asymmetry to its form, indicating a potential interaction or minor disturbance. The apparent diameter is relatively small, with a fuzzy, indistinct boundary, suggesting significant distance. 
