The galaxy presents a smooth, elliptical morphology. Its light profile appears fairly uniform, exhibiting a high degree of central concentration with a relatively low degree of surface brightness variation across its extent. The galaxy appears generally round in shape. There is no visible evidence of spiral arms, a bar, or significant dust lanes. The color index suggests a population of older stars, as indicated by the reddish-yellow hue. There is no visual evidence of tidal tails or ongoing merger activity.
