The galaxy presents as a centrally concentrated, elliptical-like system. Its light profile appears smooth with no discernible spiral arm structure. A clear bulge is visible, dominating the overall luminosity. The galaxy exhibits a yellow-orange hue, which suggests a stellar population that is composed primarily of older, redder stars. There are no obvious signs of dust lanes or active star-forming regions. The overall morphology suggests a relatively evolved galaxy with a considerable mass. There is no indication of major tidal disturbances or ongoing mergers in the immediate vicinity.
