The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, displaying a slight elongation rather than a perfectly circular form. The central region is brighter and possesses a yellowish-white hue, suggesting an older stellar population. The outer regions of the galaxy display a gradual decrease in surface brightness. There is a very subtle suggestion of blue in the disk, which indicates minimal active star formation. There are no obvious dust lanes, tidal tails, or strong distortions visible in the image.
