The galaxy presents a largely spheroidal morphology, appearing mostly smooth and relatively undisturbed. There is a high degree of central concentration, with light intensity decreasing radially outwards from a bright core. The galaxy exhibits a moderate ellipticity, tending slightly toward a round shape rather than a highly elongated or cigar-shaped form. While no distinct spiral arms or disk-like structures are readily apparent, subtle variations in color and surface brightness suggest underlying complexities in its stellar populations and dust distribution. Overall, the galaxy appears to be a fairly evolved system, possibly an elliptical galaxy or a lenticular galaxy seen at a sufficient distance to obscure finer details. The color indices imply a significant population of older stars. The galaxy is a fairly luminous object in the DESI bands, suggesting an overall large size.
