The galaxy appears to be an elliptical galaxy at a redshift of approximately 0.356. It exhibits a smooth morphology, with minimal discernible features such as spiral arms or a prominent disk. The light distribution is concentrated towards the center and gradually fades outwards. The overall shape is close to circular. There is no evidence of active galactic nuclei or signs of significant dust lanes, which contribute to its smooth appearance. It is likely a relatively massive galaxy, exhibiting a moderate rate of star formation. The galaxy shows no major disturbances or any strong indication of interaction with other galaxies. The galaxy exhibits a higher magnitude in the g-band compared to the r and z bands, suggesting it may have higher star formation regions that the other two, or other factors like metallicity could also play a role in the bluer g-band magnitude.
