This galaxy exhibits a largely smooth morphology, appearing elliptical in shape with a high degree of central concentration. The light profile suggests a dominant bulge component, with a gradual decrease in luminosity outward from the core. There is little discernible evidence of spiral arms or distinct features associated with active star formation. The color profile is relatively uniform across the galaxy, indicating an older stellar population. Some minor disturbances are possible, though the galaxy appears to be generally undisturbed. There is no indication of tidal tails or strong gravitational interactions suggesting recent or ongoing mergers. The galaxy's overall appearance is consistent with an early-type galaxy at an intermediate redshift.
