The galaxy presents a largely smooth, elliptical morphology. It appears quite symmetrical, exhibiting a centrally concentrated bright core that gradually diffuses outwards. The overall color gradient suggests a significant population of older stars, evidenced by the reddish hues, particularly in the outer regions. There is a subtle indication of a disk-like structure, but it is not well-defined; its presence is only weakly suggested by a slight flattening along one axis. The galaxy lacks prominent spiral arms or distinct dust lanes, reinforcing the interpretation of it being an elliptical type. There's a suggestion of a minor disturbance in the galaxy's shape and a hint of a possible interaction or tidal feature on its periphery, but more detailed analysis would be required to confirm it.
