This galaxy appears to be a relatively smooth, elliptical galaxy, with an approximate diameter of 8.2 kiloparsecs. The galaxy exhibits a concentrated central bulge of older stellar populations, indicated by the yellowish hue. There's a possible faint and diffused disk-like structure surrounding the bulge. No distinct spiral arms or dust lanes are visible, suggesting a lack of significant ongoing star formation. The galaxy appears to be isolated, showing no signs of tidal interactions or mergers. It is relatively round in shape. 
