This galaxy appears to be a relatively smooth, elliptical galaxy with an oblate spheroidal shape. The color profile suggests an older stellar population, with a yellowish hue indicative of fewer young, blue stars and a dominance of redder, evolved stars. There is little evidence of spiral arm structure or significant dust lanes. The galaxy exhibits a concentrated central bulge that gradually fades into its outer regions. There is no obvious evidence of active galactic nuclei activity or recent major mergers. A minor disturbance cannot be ruled out, however. Overall, the galaxy presents as a mature, early-type system that has largely completed its major star formation.