The galaxy exhibits a clear spiral structure, viewed at an oblique angle. Two prominent spiral arms emanate from the central bulge region, displaying a moderately wound morphology. The central bulge appears significant in size and exhibits a yellowish hue. Fainter spiral arms appear to be present beyond the prominent ones. The galactic disk is readily apparent and not viewed edge on. There is no obvious evidence of recent major merger activity or strong tidal disturbances. There may be a slight distortion of one of the arms, indicating a minor gravitational interaction. A bar structure appears to be present through the central bulge.
