The galaxy presents a largely smooth, elliptical morphology. It appears highly concentrated, with a bright central bulge that dominates the overall structure. The color profile suggests an older stellar population, with a reddish-yellow hue indicative of evolved stars. There is very little evidence of spiral arm structure or dust lanes. The isophotes appear relatively regular and undisturbed, suggesting a relaxed dynamical state. The overall impression is that of a massive, evolved galaxy with little ongoing star formation.
