The galaxy presents as a luminous, centrally concentrated object. The primary morphology appears to be that of a smooth, elliptical galaxy, though there is the slight suggestion of a disk component. The central bulge is a bright, yellow-white hue, indicating a population of older stars. The outer regions exhibit a gradual decrease in luminosity with no distinct spiral arm structure visible. The overall shape approximates a near-circular ellipse. There is no clear evidence of active galactic nuclei activity, major mergers, or significant tidal disturbances within the observable light. The galaxy's color suggests relatively low rates of recent star formation.
