The galaxy presents a largely smooth morphology, exhibiting a high degree of rotational symmetry. Its shape is predominantly round, with only minor deviations from a perfect circular profile. The light distribution is concentrated towards the center, with a gradual decline in surface brightness towards the outer regions. There are no obvious signs of spiral arms or a distinct disk structure. The galaxy appears to be relatively undisturbed, showing no prominent tidal features or evidence of an ongoing major merger. Subtle irregularities or minor disturbances may be present in the galaxy's morphology, hinting at possible past interactions or internal processes. The galaxy exhibits a color gradient, with bluer colors concentrated in the outer regions, suggesting the presence of younger stellar populations or ongoing star formation in those areas. The central regions appear redder, possibly indicating the presence of older, more evolved stars.
