The galaxy presents as a relatively smooth, centrally concentrated object with a somewhat elliptical morphology. The light distribution appears to be fairly uniform, lacking any distinct spiral arm structures or prominent dust lanes. There is a subtle color gradient, trending from a bluer hue towards the center to a slightly redder color in the outer regions, suggesting possible variations in stellar populations or dust content across the galaxy. The overall appearance indicates a mature system, potentially an elliptical or lenticular galaxy, without significant ongoing merger activity.
