The galaxy presents a largely smooth, elliptical morphology, exhibiting a concentrated central bulge. The galaxy's color profile indicates a population of older stars, appearing predominantly yellow with hints of red. There are minimal signs of spiral arm structure or significant dust lanes; the galaxy is largely featureless. Its overall roundness suggests a minimal rotational component. A very slight asymmetry in the galaxy's outer isophotes cannot be ruled out, though there is no clear indication of a major merger event. Some low-level star formation may be occurring, based on faint blue tinges around the edges.
