The galaxy presents an elliptical morphology, appearing generally smooth and rounded in shape. There is no prominent disk structure visible. The galaxy exhibits a dual-core structure or potential signs of interaction/merging, with two distinct centers of light concentration. The color profile reveals a redder component to the west and a bluer component to the east. The overall color suggests a developed stellar population, but the presence of bluer regions indicates ongoing or recent star formation, albeit potentially at a low rate. There is some evidence of minor tidal disturbances or asymmetries in the overall shape, possibly indicative of past gravitational interactions.
