The galaxy presents a generally smooth morphology with a high degree of elongation. It is likely an elliptical or lenticular galaxy, given the absence of discernible spiral arms or a prominent disk structure. The object exhibits a color gradient, with a central region that appears more yellow/white, suggesting an older stellar population. The outer regions are fainter and exhibit a slightly bluer hue, potentially indicating the presence of younger stars or ongoing star formation, though this is less pronounced. There is no evidence of a strong central bulge or active galactic nucleus. There is an apparent minor disturbance. The red shift indicates that the object is significantly distant.
