The galaxy presents as a relatively smooth, elliptical-like structure. The light distribution appears concentrated towards the center, which displays a slightly brighter, diffuse glow suggesting a possible core region. The outer regions of the galaxy fade gradually into the background, with no distinct, sharp edges. There is a subtle color gradient visible, with a slight shift towards bluer tones in the outer areas. The overall form exhibits a low degree of rotational symmetry, with a slightly elongated appearance, but no prominent spiral arms or other significant features are observable. There is no clear evidence of any ongoing major merger events, though some minor irregularities in the outer halo are suggested.
