The galaxy presents a predominantly smooth morphology, characteristic of an elliptical or S0 type. The light distribution appears concentrated toward the center, indicating a prominent bulge. The galaxy exhibits a subtly elongated, though mostly rounded, shape. Color gradients suggest an older stellar population, with a yellowish hue dominating the central region. There is no discernible dust lane or spiral arm structure. Faint outer regions indicate a less concentrated, diffuse halo. Based on the estimated redshift, this object is a galaxy observed in the distant universe. The galaxy does not appear to be undergoing any major merger activity, with only slight hints of disturbance in its overall structure. The lack of distinct features suggests that star formation activity is relatively quiescent.