The galaxy presents as a relatively smooth, elliptical structure with a distinct central bulge. Its overall shape is elongated, exhibiting a cigar-like appearance. There is a noticeable color gradient, transitioning from a bright, yellowish-white core to a bluer, more diffuse halo. The galaxy lacks any readily discernible spiral arms or distinct dust lanes. There are no clear indications of major mergers or significant tidal disturbances. Faint and diffuse outer regions indicate some extended stellar population beyond the main body.
