This galaxy appears to be a relatively smooth, elliptical or lenticular system at a redshift of approximately 0.22, indicating a substantial distance. It presents with a generally featureless morphology, lacking any readily discernible spiral arms or bar structures. The galaxy exhibits a centrally concentrated luminosity profile with a peak in yellow wavelengths, suggesting an older stellar population and relatively low levels of on-going star formation within the nucleus. The outer regions show a gradual decrease in brightness and appear slightly bluer, indicating a possible trace amount of younger stars residing in the outskirts. There is a slight elongation of the galaxy’s overall shape, but its morphology appears predominantly spheroidal, closer to a classical elliptical. The overall impression is of a passively evolving system with a considerable stellar mass. There are very minor, if any, signs of any disturbances or recent mergers.
