The galaxy presents a generally smooth, elliptical morphology. It appears largely featureless, with a dominant central bulge that gradually diffuses outward. The light distribution suggests a relatively high degree of rotational symmetry. The color profile is somewhat complex. The central region exhibits a bright, whitish-yellow hue, transitioning to a faint bluish tone in the outer regions. This color gradient suggests the presence of a relatively old stellar population in the core, with possible ongoing star formation in the outer regions. There is some asymmetry in the bottom of the galaxy, with some green color, which could suggest some star formation. No distinct spiral arms or bar structures are evident in the visible light. Overall, the galaxy appears to be an elliptical galaxy nearing the late stages of its evolution, with only minor disturbances and no significant ongoing mergers.
