The galaxy presents a generally smooth morphology. It appears as a slightly elongated, centrally concentrated object, likely a spheroid. The core region exhibits a bright, luminous yellow-white glow, indicating a high concentration of stars. The outer regions gradually fade into a more diffuse, bluish halo. There is no obvious spiral structure or pronounced disk component visible. Faint irregularities may suggest minor disturbances in the galaxy's structure, but overall it appears relatively undisturbed, and does not show strong signs of on-going merger activity. The colour profile suggests that the central bulge contains older stellar populations, while the fainter, bluer outskirts could indicate some ongoing, albeit low-level, star formation. The galaxy's morphology is consistent with an elliptical galaxy at intermediate redshift.
