The galaxy appears to be a relatively smooth, early-type spiral galaxy, likely somewhere between an elliptical and a spiral. The central bulge is prominent and appears yellowish in color, suggesting an older stellar population. Fainter, bluish spiral arms are visible, but they are not well-defined, and may contain areas of new star formation. The overall structure seems undisturbed, with no obvious signs of a major ongoing merger, though some minor asymmetries or disturbances cannot be ruled out. The galaxy is nearly circular in appearance. The light distribution is centrally concentrated, gradually fading towards the outer regions.
