The galaxy presents as a diffuse, centrally concentrated object. The overall morphology appears largely smooth with some subtle features or hints of a disk-like structure, although it is difficult to definitively resolve spiral arms or a distinct bar. The shape is generally round, with a slight deviation from perfect circularity. There are indications of potential minor disturbances in the outer regions of the galaxy, however no major mergers are apparent, and the system looks like it has been mostly undisturbed for some time. The galaxy displays a central bulge that is well-defined and prominent, as well as a significant amount of ongoing star formation.
