The galaxy presents as a centrally concentrated object with a generally smooth morphology, showing a high degree of circularity. The light profile appears relatively uniform, transitioning gradually from the core to the outer regions. The core exhibits a yellowish-white hue, suggesting a population of older stars. Surrounding this is a more diffuse region of redder coloration, potentially indicating the presence of a population of evolved stars or dust obscuration. There is no readily apparent structure such as spiral arms or a distinct bulge. The galaxy does not appear to be undergoing any major mergers or disturbances based on the image. Overall, the galaxy's appearance is consistent with that of an elliptical galaxy.
