The galaxy presents as a relatively smooth object, with a centrally concentrated morphology. Its overall shape appears somewhat elliptical, approaching a circular form. There is a suggestion of a weak disk-like structure but the image quality limits further analysis. The galaxy's color gradient indicates a population of older stars, but with ongoing, albeit modest, star formation. No major disturbances are visible, suggesting it is not currently undergoing a major merger. However, there might be a hint of a minor disturbance.
