The galaxy presents as a centrally concentrated, somewhat elliptical, and relatively smooth structure. It appears largely featureless. The core region exhibits a yellow-white hue, suggesting a population of older stars. Moving outward from the core, there is a diffuse, blueish halo indicating the presence of younger, hotter stars. There appears to be a slight disturbance on the outskirts of the blueish halo. Overall, the galaxy does not appear to be actively merging, though there may be a minor disturbance occurring. Based on the overall shape, it is likely an elliptical galaxy.
