The galaxy presents as a relatively smooth, elongated structure. It exhibits a central bulge that appears yellowish-white, indicating a concentration of older stellar populations. Surrounding the bulge is a fainter, bluer disk. This suggests ongoing or recent star formation within the disk. The overall morphology indicates a possible elliptical galaxy, however, the subtle bluer halo could signify the existence of a spiral disk that is being viewed nearly edge-on. There appear to be no major disturbances or signs of on-going merging events and no tidal tails or other obvious deformities in the galaxy's structure. 
