The galaxy presents as an elongated, moderately inclined spiral or lenticular galaxy with a central bulge that appears relatively smooth and concentrated, with a high Sersic index value. The blue hue in the galactic disk suggests ongoing star formation. Morphological classifications from citizen scientists suggest that the galaxy exhibits some signs of minor disturbances or merging, although none seem to be prominently visible in the image. Its estimated mass suggests a relatively normal sized galaxy. The estimated star formation rate also suggests a typically star forming galaxy.
