The galaxy presents a largely smooth and centralized structure, indicative of an elliptical morphology, though some disk-like qualities are present. The core exhibits a bright, concentrated luminosity, which gradually diffuses outwards. The overall color profile appears redder, particularly in the central region, suggesting a relatively older stellar population. The shape is somewhere between round and oblong. There is no clear evidence of significant spiral arm structure or strong dust lanes, and no signs of tidal tails or morphological disturbances indicative of recent major mergers, though minor disturbances cannot be ruled out. 
