The galaxy appears as a single, somewhat diffuse object with a concentrated central region. The color is primarily a yellowish-white, suggesting an older stellar population with fewer hot, young stars. There is a slight elongation with a high degree of axial symmetry. No prominent spiral arms or dust lanes are clearly visible. The overall morphology is smooth and featureless, indicative of an elliptical galaxy or a lenticular galaxy with a dominant bulge component. There are no indications of recent major mergers or tidal disturbances. The galaxy exhibits a gradual decline in brightness from the core to its outer edges.
