The galaxy presents as a somewhat diffuse object, elongated in shape, with a brighter central region suggesting a galactic bulge. The color gradient shifts subtly from a bluer hue near the center outwards, possibly indicating younger stellar populations in the core and relatively older stars in the outer regions. There is a slight asymmetry in the overall structure, with a hint of disturbed morphology; it might be the result of a minor gravitational interaction. Indications suggest moderate levels of current or recent star formation. The galaxy shows no defined spiral arm structure, but rather a more amorphous shape.
