The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a slightly elliptical morphology, appearing more rounded than elongated. The primary color is a yellowish-white, suggesting a dominant population of older stars. There is a subtle gradient in color, with the central region appearing slightly more yellow and the outer regions exhibiting a faint bluish tinge, which might indicate some ongoing, but low-level, star formation in the outer regions. No distinct spiral arm structures or a prominent galactic disk are visually apparent. There is no evidence of a major ongoing merger or tidal disruptions in the image; however, there may be a very faint minor disturbance. The lack of significant dust lanes or patchy extinction further supports its classification as a relatively evolved system.
