This galaxy exhibits a disc-like morphology with notable spiral arm structures. Two or three primary spiral arms can be distinguished. The arms appear relatively tightly wound near the central bulge region, gradually becoming looser further out. A moderate bulge is visible but doesn't dominate the overall structure. The galaxy does not appear to be undergoing a major merger, but minor disturbances may be present. It's a fairly face-on spiral, rather than edge on. The light emitted from this galaxy tends to be in the bluer wavelengths.