The galaxy presents a largely smooth and elliptical morphology. It exhibits a concentrated central bulge, appearing yellow in color, with a slightly more diffuse halo. While the galaxy appears mostly smooth, there is some evidence of a faint, extended structure suggesting a possible disk component, which is faint and inclined relative to our line of sight. This galaxy has no clear signs of active star formation, and appears to be a relatively quiescent system. The overall structure implies an evolved system, likely with a significant population of older stars. There appears to be no indications of major mergers or tidal disturbances. The round shape of the galaxy suggests that it is probably an elliptical galaxy, with a stellar mass of likely over 100 billion times the mass of the sun.
