The galaxy presents as a face-on spiral type, though the morphology is somewhat obscured. Faint, blue-tinged spiral arms appear to emerge from a central bulge. A moderate bulge size seems evident, with a luminosity gradient decreasing smoothly from the center outwards. The arms are not sharply defined, suggesting a flocculent or grand design spiral structure that is either highly disrupted or relatively diffuse. There is no obvious bar structure visible in the image. The object appears relatively isolated, with no clear signs of major mergers or significant tidal disturbances. The overall color suggests ongoing, but perhaps not vigorous, star formation within the spiral arms, indicated by their blue hue. The low redshift suggests it is a relatively nearby galaxy.
