This galaxy presents as a luminous, relatively smooth object. Its morphology suggests a spheroid-dominated system, possibly an elliptical or lenticular galaxy. The galaxy exhibits a radial color gradient, appearing more yellow toward the center and exhibiting bluer hues in its outer regions. This may indicate an older stellar population concentrated towards the nucleus with younger stars in the outskirts. There may be some minor irregularity in the morphology that may be due to an ongoing interaction or merger. The object appears largely undisturbed and the galaxy is most likely in a stable state.