The galaxy appears to be a spiral type. The galaxy is relatively small and the light is somewhat diffuse. It is more luminous in what appears to be the redder bands, and there are some light variations and features that could be spiral arms. There are several faint tidal tails that are visible surrounding the galaxy, suggesting it could be undergoing a minor merger. There does not appear to be a very defined central bulge or spherical component; the morphology is dominated by a relatively smooth, elongated disk structure. Overall, the galaxy exhibits characteristics consistent with a spiral galaxy experiencing possible interactions.
