The galaxy presents as a relatively smooth, elliptical structure, exhibiting a concentrated central bulge. There is a subtle color gradient visible, with the core region appearing more yellow-white, suggesting a population of older, cooler stars. The outer regions of the galaxy fade gently into the background, indicating a lack of significant star formation. There are no readily apparent spiral arms or dust lanes in the visible spectrum. The overall morphology suggests an evolved system, likely an elliptical galaxy with a substantial stellar mass, and very low ongoing star formation rate. The galaxy exhibits a high degree of symmetry, and does not show any visible signs of recent tidal interactions or major mergers.
