This galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that transitions smoothly into an extended halo. The galaxy's color profile suggests a population of older stars, with a dominant yellowish hue. There is no immediately apparent evidence of spiral arm structure or significant dust lanes. The galaxy displays a nearly circular morphology, showing little deviation from a rounded shape. No signs of ongoing or recent major merger events are detectable in this image, however, subtle disturbances cannot be ruled out. The overall appearance of the galaxy is indicative of a mature, passively evolving system.
