The galaxy presents a somewhat smooth, elliptical morphology with a bright, concentrated central bulge. The overall color gradient transitions from a yellowish-white core to a redder, more diffuse outer region. This reddening suggests a stellar population with a significant proportion of older, cooler stars in the outer regions, relative to the core. There is a hint of a faint, disklike structure, but it is not clearly defined, and the galaxy is largely spheroidal. There are no obvious signs of active star formation regions or significant dust lanes. There is a very subtle asymmetry, and the galaxy may be undergoing a minor interaction. 
