The galaxy appears as a faint, elongated structure. It is likely a spiral galaxy viewed edge-on. There is no pronounced central bulge, implying it is likely a late-type spiral. The luminosity in the g-band appears relatively faint, with a brighter luminosity in the redder bands, so that suggests significant stellar populations are present in the older redder stars. Its elongated shape suggests that any spiral arms are tightly wound or indiscernible at this resolution.
