The galaxy presents as a relatively compact structure, with a somewhat diffuse appearance and a moderate central brightness concentration. It appears to be a lenticular or early-type spiral galaxy at an approximate distance of 220 megaparsecs (based on its redshift). The galaxy does not show any obvious spiral arm structure or prominent dust lanes. There are subtle hints of disturbed morphology, possibly indicating minor gravitational interactions or a past merger event, although the image quality limits definitive conclusions. Color gradients suggest that there may be a central bulge with an older stellar population and a more extended disk component. Overall, this is a fairly quiescent galaxy with a low estimated star formation rate, typical of galaxies in this mass range at this redshift.
