The galaxy presents as a spiral, observed at a moderate inclination. Its apparent size suggests that it is a reasonably large galaxy. The spiral arms appear to be loosely wound, extending outwards from a slightly elongated central bulge. The arms exhibit a relatively smooth structure, with some mottling indicating regions of star formation. The central bulge appears moderately bright with a yellow-orange hue suggesting an older stellar population. The outer spiral arms appear to be bluer in color, consistent with younger, hotter stars. There is evidence of two distinct arms. There are no obvious signs of any major mergers or significant tidal disturbances. The galaxy is likely undergoing modest levels of star formation.
