The galaxy presents as an elliptical morphology, with a smooth, centralized luminosity profile. The core exhibits a bright, yellowish-white hue, suggesting a concentration of older stellar populations and potentially a supermassive black hole actively accreting material. Moving outwards, the galaxy transitions to a fainter, reddish-orange color. This suggests the presence of a more dispersed, older stellar population at the galaxy's periphery. There is no visual evidence of spiral arms, dust lanes, or active star-forming regions. The overall structure appears largely undisturbed, showing no signs of major recent mergers or tidal interactions. The ellipticity appears modest. The galaxy is reasonably compact.
