The object presents as a moderately luminous galaxy at a redshift of approximately 0.168, indicating a significant distance. Its morphology appears largely smooth and elliptical, with a high degree of central concentration. The color gradient transitions from a yellowish-white core to a bluer outer halo. There are no visually discernible spiral arms or significant dust lanes visible within the image. The shape is generally rounded with some slight ellipticity. No major interactions or merging events are immediately evident, although there may be some signs of minor disturbances in the outskirts. Based on the observed color and morphology, the galaxy likely hosts an older stellar population, with relatively low ongoing star formation. 
