The galaxy presents as a lenticular or early-type spiral galaxy, exhibiting a significant central bulge that appears relatively smooth and featureless in this image. The disk component, while present, is not as pronounced as in later-type spirals. Some subtle asymmetry or minor disturbances are potentially present, but the galaxy overall exhibits a relatively settled morphology. The galaxy's light profile transitions smoothly from the bright nucleus outwards, suggesting a stable stellar population distribution. There is a slight elongation in the galaxy's shape, tending towards an in between roundedness. A color gradient is observed, with the core appearing more yellowish, possibly indicating a higher concentration of older, redder stars in the bulge, and the outer regions appear bluer, which is suggestive of some ongoing, albeit limited, star formation. This is consistent with the observed redshift of z=0.22, placing it at a considerable distance.
