The galaxy presents as a relatively smooth, centrally concentrated object. The color profile suggests an older stellar population, with a dominant yellow hue across the primary structure. The morphology appears elliptical, exhibiting a slight elongation. There is no clear spiral arm structure visible, nor any significant dust lane obscuration or other signs of active star formation regions. The outer regions of the galaxy fade smoothly into the background sky, indicating a gradual decrease in stellar density with increasing radius from the galactic center. There is only a slight hint of any tidal disturbances or interactions. The galaxy appears to be isolated and undisturbed.
