The galaxy presents as a centrally concentrated, elliptical morphology. Its core exhibits a bright, yellowish hue, suggesting a high density of older stellar populations. Moving outward from the core, the color profile subtly shifts toward a bluer tint, indicating the presence of younger stars. The overall smoothness and roundness of the galaxy are prominent characteristics, though there is subtle indication of minor disturbance that may suggest interaction. The galaxy has a fairly diffuse nature to it, with its edges fading gently into the background, rather than showing any hard edges. There is no visual evidence of a strong spiral structure or prominent dust lanes.
