The galaxy presents as a largely smooth, elliptical object. It exhibits a concentrated, bright core that diminishes gradually into its outer regions. The color profile suggests an older stellar population, with a dominant yellowish hue in the core, transitioning to redder tones towards the outer edges. There is no apparent evidence of spiral arm structure or significant dust lanes. The overall shape is approximately circular, exhibiting minimal signs of distortion or interaction with other galaxies. The outer regions are more diffuse. 
