The galaxy presents as a singular, relatively compact object. The overall color profile appears to be a greenish white, suggesting a population of intermediate age stars. The light distribution is mostly concentrated at the center, indicating a prominent bulge. The object has an elliptical appearance. There is some indication of possible disturbance or tidal features, but the dominant morphology is consistent with a smooth, non-disk galaxy. Although a merger cannot be ruled out entirely, there is nothing to confirm that it is occurring or has occurred.
