This galaxy presents a primarily smooth, elliptical morphology. It exhibits a bright, concentrated central bulge region that transitions outwards into a less luminous halo. A subtle disk component is potentially observable, though heavily obscured. The color profile indicates a general population of older stars, based on the apparent yellow to reddish hues, with a hint of possible ongoing star formation due to some bluer regions interspersed within its outer structure. There is no visually apparent indication of any major mergers or tidal disturbances in this galaxy. The overall structure suggests a galaxy that has largely completed its morphological evolution into a spheroid-dominated system.
