The galaxy appears to be a smooth, elliptical system. It exhibits a centrally concentrated bulge that is notably brighter and more yellow than the surrounding halo. The galaxy's morphology suggests an evolved system with a dominant spheroid component. There is no clear evidence of spiral arms or significant dust lanes. The outer regions fade gradually into the background sky, with a slight elongation, but no major disturbances in its structure, which indicates it may be a disk galaxy. No evidence of significant tidal interactions or ongoing mergers are seen. The galaxy's overall color gradient indicates a relatively older stellar population, with the redder central regions suggesting a higher concentration of older stars. Star formation appears to be low.
