The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is elliptical, appearing mostly round with only a slight deviation from perfect circularity. A central bulge dominates the galaxy's structure, exhibiting a bright, yellowish-white hue suggestive of an older stellar population. There is a very faint hint of a disk structure. No prominent spiral arms or dust lanes are visible. There is a small chance of minor gravitational disturbance, but overall the galaxy appears unperturbed, without significant tidal features or evidence of a recent major merger. 
