The galaxy presents as a somewhat smooth, centrally concentrated object. It exhibits a slightly elongated, oblate shape, appearing neither perfectly spherical nor highly flattened. There is a subtle hint of a disk-like structure or faint spiral arms, but they are not well-defined. Color gradients suggest a relatively evolved stellar population. The central bulge appears slightly brighter and yellower, possibly indicating a higher concentration of older stars. The galaxy shows some signs of possible disturbance, but no major merger is taking place. Overall, the galaxy appears relatively isolated.
