The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely elliptical, exhibiting a high degree of roundness with only a slight deviation from perfect circular symmetry. There is no prominent disk structure visible. The central region displays a bright, luminous core which gradually diffuses outwards. A color gradient is observed, with the core exhibiting a yellowish-white hue, suggesting an older stellar population. Fainter, bluer colors are seen in the outer regions, potentially indicating regions of more recent star formation, albeit at a low rate. There is no evidence of major mergers or significant tidal disturbances in the immediate vicinity. The overall appearance indicates a galaxy that is potentially passively evolving with a relatively old stellar population.
