The galaxy appears to be a spiral, viewed at a moderate angle, potentially intermediate between edge-on and face-on. There is evidence of a central bulge, somewhat indistinct, with a yellowish-white hue. The spiral arms are not well-defined, appearing somewhat flocculent. One arm seems to show some blue star formation regions, as indicated by the presence of blue light. The galaxy appears moderately bright. There may be some dust lanes visible within the galaxy, but the resolution limits a clear identification of these features. The galaxy does not appear to be undergoing a major merger, although there may be minor tidal disturbances visible along the outer edges. The overall morphology could be considered weakly barred.
