The galaxy presents as a relatively smooth, centrally concentrated structure. It appears somewhat elliptical, displaying an intermediate axis ratio. There is a subtle color gradient, transitioning from a bluer core region to redder outer regions, indicating a variation in stellar populations. It has very few disk like structures. There is no sign of major mergers. The absence of prominent features like spiral arms or dust lanes suggests a more evolved system. Based on visual inspection, there may be some signs of minor interactions with other objects or slight asymmetry, suggesting a dynamically active environment.
