The galaxy presents as a relatively smooth, elliptical-like structure. The central bulge is quite prominent, exhibiting a high degree of luminosity. The galaxy appears to be generally lenticular in shape, not precisely spherical, but more of an oblate spheroid. There is a slight indication of a disk-like structure extending outward from the central bulge, however it is difficult to fully ascertain with this observation. The overall color of the galaxy appears to be somewhat redder, indicating a stellar population that is relatively old. There are minimal signs of dust lanes or active star formation regions based on this observation. There are no clear indications of a major merger event or significant tidal disturbances, although a slight asymmetry to the outer halo might be present. Overall, the morphology suggests a relatively quiescent galaxy.
