This galaxy presents as a somewhat smooth, centrally concentrated object, with a distinct but not sharply defined nucleus. The morphology appears to be disk-like, with a suggestion of a flattened structure. The color profile shifts from a bluer hue in the outer regions to a more red-toned center. There is a lack of well-defined spiral arms, suggesting a later-type spiral galaxy or potentially a lenticular galaxy. Some slight disturbances can be observed, possibly due to minor mergers. It is likely a relatively massive galaxy, forming new stars at a moderate rate.
