The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge that is noticeably bright and yellow in color, suggesting an older stellar population dominated by evolved stars. The galaxy appears largely featureless, with little evidence of spiral arms or significant dust lanes. The outer regions of the galaxy appear fainter and more diffuse, with a gradual decrease in surface brightness from the center outwards. The overall shape appears round, with no obvious signs of significant tidal distortion or ongoing merger activity. The color gradient indicates a possible radial change in stellar populations, with the central region being redder than the outer regions. The high degree of smoothness observed suggests a system that has undergone significant dynamical relaxation.
