This galaxy presents as a relatively smooth, centrally concentrated object. The color gradient suggests a dominant older stellar population, with a possible enhancement of ongoing star formation, or perhaps a more dust-obscured region, centrally located. The morphology appears largely undisturbed with no immediately obvious signs of tidal features or a major merger event. The galaxy appears to be in an early stage of transitioning into an elliptical morphology, given it is still slightly disk like, but does not contain a significant disk.
