The galaxy exhibits a morphology that leans towards being smooth and relatively undisturbed. It appears somewhat elliptical, with a noticeable but subtle elongation along one axis. The central region is bright and concentrated, suggesting a significant stellar density and potentially a supermassive black hole actively accreting matter. The galaxy's color profile indicates a population of older stars dominating the light output, as evidenced by the reddish-yellow hue, though there may be some ongoing, albeit subdued, star formation contributing to a slightly bluer component in the outer regions. There is a hint of a disk-like structure with minimal features. The overall structure is coherent, showing no obvious signs of ongoing major mergers, although a slight asymmetry could indicate a past minor interaction or accretion event.
