The galaxy presents a generally smooth, elliptical morphology. The light distribution suggests a central concentration of older stars, indicated by the yellowish hue in the core region. Progressing outwards, the color appears to become slightly bluer, suggestive of a younger stellar population in the outer regions, although this effect is subtle. There is little evidence of spiral arms or dust lanes. Overall, the galaxy's structure appears relatively undisturbed, showing no signs of major mergers, although a very faint asymmetry in the outer halo might suggest a minor interaction. The galaxy's moderate redshift indicates it's a relatively distant object. There's a hint of ongoing, albeit low-level, star formation. The galaxy is not perfectly spherical, displaying a slightly elongated shape.
