The galaxy presents as a generally smooth, elliptical structure. It displays a distinct central bulge region exhibiting a yellowish-orange hue, possibly indicating an older stellar population. Surrounding the central bulge is a more diffuse, greenish halo. This halo structure suggests the presence of a younger, bluer stellar population and possibly ongoing star formation. The overall shape appears moderately elliptical, with an axial ratio suggesting it is not perfectly spherical. There is no clear evidence of spiral arms or a bar structure. There are no obvious signs of major mergers or tidal disturbances. However, a minor asymmetry cannot be ruled out. The galaxy appears relatively isolated within the observed field.
