This galaxy presents as a relatively smooth, lens-shaped object with a noticeable central bulge. The color profile suggests a concentration of older stars in the bulge, giving it a yellowish hue, and a slight inclination. There is a hint of a disk structure present, with bluer colors toward the edges of the galaxy, which might imply more recent star formation. The galaxy doesn't exhibit any obvious signs of recent major merger activity but there are some minor disturbances observed in the image. The light is centrally concentrated, indicating a high degree of radial symmetry. The galaxy appears to be fairly isolated.
