The galaxy presents as a fairly well-defined elliptical structure. The central region exhibits a significant concentration of light, suggesting a prominent galactic nucleus. A noticeable colour gradient exists, shifting from a bluer core to redder outer regions, possibly indicative of varying stellar populations and ongoing star formation. Overall, the galaxy's profile appears smooth and somewhat elongated with a slight flattening, revealing a non-negligible ellipticity. Based on the colours, it can be determined that the galaxy is an intermediate redshift.
