The galaxy presents as a centrally concentrated object with a generally smooth appearance. Its morphology is largely elliptical, appearing mostly round, with only minor deviations from a perfectly circular shape. There is evidence of some substructure and potential minor disturbances, but the overall appearance suggests a relatively relaxed and well-mixed system. The galaxy exhibits a color gradient, appearing somewhat bluer in the outer regions and redder toward the core. This suggests a population of younger, hotter stars in the periphery and older, cooler stars concentrated toward the center. There may be some weak tidal features or faint shells visible upon closer inspection, indicative of past minor mergers or interactions. The light is moderately bright. No obvious spiral arms or distinct disk features are apparent. 
