The galaxy presents as a centrally concentrated, smooth structure with a high degree of radial symmetry. It appears elliptical in shape, exhibiting a near-spherical morphology. The core region displays a yellowish hue, suggesting an older stellar population. The outer regions exhibit a faint blue tinge and diffuse halo, perhaps indicating a small amount of on-going star formation, but the overall star formation rate is relatively low. There is no obvious indication of spiral arms or a distinct galactic disk. No signs of tidal disturbances or major mergers are apparent from this image, although very minor disturbances could be present. The overall luminosity suggests this is a massive galaxy.
