The galaxy presents as a relatively smooth, elliptical morphology. It appears to be a flattened spheroid, exhibiting a distinct central bulge that gradually fades into a more diffuse halo. The dominant color is a yellowish-orange hue, suggesting a stellar population comprised primarily of older, evolved stars. There is little evidence of significant dust lanes or spiral arm structures, indicative of a lack of ongoing active star formation. The overall appearance is consistent with a mature elliptical galaxy, likely residing in a relatively quiescent environment.
