The galaxy presents a generally smooth morphology. It exhibits a bright, concentrated central region or bulge. The overall shape appears elliptical, displaying an intermediate roundedness, with only a slight elongation. The galaxy's color suggests a relatively evolved stellar population. There is no clear evidence of significant spiral arm structure or active star formation regions. Furthermore, there are no obvious signs of major mergers or significant tidal disturbances in the immediate vicinity. Faint, diffuse light extends outwards from the central region indicating a halo.
