The galaxy presents as a relatively smooth, elliptical morphology with a slightly elongated shape. It exhibits a concentrated central bulge that appears yellowish-white, suggesting an older stellar population. The outer regions of the galaxy display a bluer hue, possibly indicating more recent, albeit modest, star formation activity. There is no apparent evidence of spiral arms or a distinct disk structure. The galaxy shows no significant signs of ongoing mergers or major disturbances, maintaining a largely undisturbed form. The overall appearance points to a galaxy in a relatively quiescent state.
