The galaxy presents as an elliptical-like structure, with a high degree of central concentration. Its morphology appears predominantly smooth, lacking discernible spiral arms or prominent dust lanes. The light distribution suggests a relatively spherical shape, with only slight deviations from perfect roundness. No clear signs of ongoing major mergers or significant tidal disturbances are immediately evident. The galaxy displays a smooth radial profile, where brightness decreases with distance from the galactic center. The colour index suggests a galaxy population comprised of evolved stars, likely corresponding to an older stellar population. The observed colour is characteristic of a galaxy with suppressed or quiescent star formation, potentially indicating that star formation activity is low.
