The object appears to be a galaxy at a considerable distance. The central region is moderately concentrated but diffuse, exhibiting a smooth morphology with a slight elongation. There is a faint indication of potential tidal features or a minor disturbance in its outer regions, suggesting a possible interaction or merger history. The galaxy exhibits a faint, bluish tint, potentially indicating moderate star formation. The overall structure does not present a well-defined disk or spiral arms, lending evidence towards a more spheroidal or irregular shape. Further spectroscopic analysis is needed to confirm redshift and internal kinematics.
