The galaxy presents as a predominantly smooth, elliptical structure. Its overall color appears yellowish-orange, suggesting a population dominated by older stars with lower rates of ongoing star formation. There is a slight elongation visible, though the galaxy is largely circular in its apparent shape. There are no obvious signs of strong tidal distortions or major mergers, although subtle asymmetries may indicate minor past interactions. The light distribution within the galaxy is centrally concentrated, with a gradual decrease in intensity towards the outer regions.
