The galaxy presents as a centrally concentrated object with a generally smooth morphology. It appears largely elliptical, with minimal disk-like features or spiral arms visible within the resolution constraints of the image. There is evidence of a bright central bulge that dominates the overall light profile. Faint color variations can be discerned, with a suggestion of bluer regions interspersed within the otherwise yellowish-white central area. No prominent dust lanes or regions of active star formation are immediately evident. Overall, the galaxy seems to be relatively undisturbed, with no major signs of ongoing mergers or tidal interactions. Based on the apparent color and morphology, the galaxy may be comprised primarily of older stellar populations.
