The object appears to be a galaxy at a moderate redshift, estimated around 0.17. It presents a generally smooth, elliptical morphology with a high degree of roundness. There is little evidence of significant disk-like structures or ongoing merging events, with only minor potential disturbances. The galaxy has a clear central concentration, fading outwards into a more diffuse halo. Color gradients suggest a relatively older stellar population dominating the central regions, while the outer regions may contain more recent stellar formation activity. The luminosity indicates a relatively large and massive galaxy.
