The galaxy appears as a single, relatively smooth object. It exhibits a generally elliptical shape with a hint of disklike structure, with a high degree of central concentration. Color gradients are subtle, transitioning from a pale, almost white core to a slightly more yellow-orange periphery. The lack of distinct features suggests a population of older stars. There is no readily apparent dust lane or spiral arm structure. The galaxy exhibits little signs of ongoing merger activity. The absence of distinct star-forming regions or blue colors indicates a relatively low specific star formation rate.
