The galaxy presents as a generally smooth, centrally concentrated light distribution. Its morphology appears primarily elliptical, with a moderate ellipticity, but with a shape more tending towards round than cigar-shaped. There is no strong evidence of spiral arm structure or a prominent disk component. No apparent major disturbances and there are not obvious signs of a recent major merger. There is a slight indication of minor disturbances present. The galaxy's color is broadly red, with the central region appearing more yellow, suggesting an older stellar population. There is a faint, diffuse halo or envelope surrounding the brighter central region.
