The galaxy presents as a centrally concentrated object, exhibiting a generally smooth morphology. Its shape appears somewhat elliptical, deviating slightly from perfect circularity. Color gradients are observable, with the central region showing a bluer hue, suggesting the presence of relatively young stars or active star formation. Towards the outer regions, the galaxy becomes redder, potentially indicating an older stellar population. There is no obvious presence of spiral arms or a distinct disk component. Furthermore, there are no clear signs of major mergers or significant tidal disturbances affecting the galaxy's structure.
