The galaxy presents as a centrally concentrated object, exhibiting a largely smooth morphology. There is a subtle hint of a disk-like structure, though the dominant characteristic is its overall smoothness. The central region displays a yellowish hue, indicative of a population of older stars. Moving outwards from the core, a slight color gradient is visible, with a shift towards bluer tones suggesting the presence of younger stars, albeit to a lesser extent. The galaxy appears relatively undisturbed, with no obvious signs of ongoing major mergers or tidal interactions. The overall shape appears close to round, with only a minor deviation from perfect circularity.
