The galaxy presents as a centrally concentrated, relatively smooth object. The light profile appears fairly symmetrical, exhibiting a near-circular morphology with a minor deviation towards a slightly elongated shape. The core exhibits a bright, yellowish hue that diffuses outwards into a subtle greenish halo. There is no immediately obvious evidence of spiral arm structure or significant dust lanes within the available resolution, suggesting a system dominated by older stellar populations. There is a very subtle hint of minor disturbance in the surrounding area.
