The galaxy presents a largely smooth morphology, displaying a high degree of central concentration. It appears nearly spherical, with a lack of discernible spiral arms or a defined disk structure. The light distribution transitions smoothly from a bright, intensely luminous core outward to a more diffuse halo. The galaxy exhibits a red-shifted color profile, indicative of a population dominated by older stars and a relatively low rate of ongoing star formation. There is no evidence of major disturbances due to mergers or tidal interactions; however, subtle irregularities in the outer regions of the galaxy cannot be ruled out due to image resolution. The overall impression is that of a massive elliptical galaxy at an intermediate redshift.
