The galaxy appears to be an elliptical galaxy, exhibiting a smooth, concentrated morphology with a centrally brightened core. Its overall shape is approximately round. There is a slight color gradient visible, with the central region appearing more yellow, which may suggest a population of older stars. The outer regions fade gradually into the background, exhibiting a bluish hue. This could be a result of small amounts of younger stars. There is no obvious spiral structure or dust lanes visible. There are no signs of any major tidal disturbances or ongoing mergers.