This galaxy appears to be an elliptical or lenticular type, displaying a largely smooth morphology. Its overall shape is predominantly rounded, though a slight elongation is observed, giving it an intermediate shape. The galaxy exhibits a color gradient, with a brighter, more yellow-orange core region and a fainter, bluer outer halo. There is no discernible spiral structure. The absence of distinct features suggests a relatively low star formation rate. There is a low probability of a major merger event, with a high probability that the shape observed is undisturbed. This system appears to be quite massive, which would likely reduce current star formation.
