This galaxy appears to be an elliptical galaxy. It exhibits a smooth, centrally concentrated light distribution with a somewhat elongated morphology. The light profile suggests a bulge-dominated system. There is no evidence of spiral arms or significant dust lanes. Color gradients suggest a population of older stars, more concentrated toward the center. No signs of major mergers are visible, though a slight asymmetry in the outer regions could indicate a minor interaction or past disturbance. The galaxy appears relatively isolated.
