The galaxy presents as a relatively smooth, elliptical morphology, with a high degree of roundness. There's a bright central bulge that fades outward to a diffuse halo. The color profile suggests an older stellar population, with a dominant yellowish-white hue in the central region, transitioning to bluish tones in the outer regions, indicating a possible gradient in stellar age or composition. There is no apparent spiral structure or dust lanes visible. The overall light distribution is concentrated towards the center, suggesting little ongoing star formation. No signs of major mergers or tidal disturbances are readily apparent, indicating a relatively undisturbed evolutionary history.
