The galaxy presents as a relatively compact structure with an apparent smooth morphology. There appears to be a bright central bulge or core, surrounded by a less luminous and more diffuse halo or disk. Hints of bluer colors in the outer regions suggest the presence of younger stellar populations possibly indicating star formation, though subdued. The overall shape appears elliptical or somewhat rounded, lacking any clear spiral arm structure or strong tidal features, perhaps minor disturbances. The red shift measurement indicates that this galaxy is at an appreciable cosmological distance, likely billions of light years.
