The object appears to be a galaxy, presenting a somewhat amorphous, disturbed morphology, potentially indicating an ongoing or recent merger event. There is a central, concentrated region of luminosity, displaying a smoother structure. This central area has an apparent yellowish hue. Adjacent to this bright center, another region, with a more diffuse and reddish color, can be observed. This may represent regions of older stellar populations or dust obscuration. The overall shape is not distinctly spiral or elliptical. Faint extensions or tidal features may be present, but these are not very pronounced. The galaxy is estimated to have an observed size corresponding to several kiloparsecs in diameter, and the spectral properties suggest a likely intermediate redshift, positioning the galaxy at a significant cosmological distance.
