The galaxy appears to be an elliptical galaxy. It presents as a relatively smooth, concentrated distribution of light, elongated in shape. There is no apparent spiral structure. The color profile suggests a population of older stars, emitting more light in the redder wavelengths. There is a subtle color gradient from the center to the outer regions, with the central area appearing slightly yellower and possibly composed of relatively older stars. No signs of active galactic nuclei or strong star forming regions can be seen, given the smooth appearance. Small indications of disturbance could be present, but the smoothness indicates a relaxed object overall. The elongation could be caused by rotation.
