The galaxy presents as a relatively smooth, elliptical structure, exhibiting a concentrated central bulge that graduates outward to a less defined halo. The core region is characterized by a yellowish-white hue, suggesting an older stellar population with minimal ongoing star formation. The outer regions, although faint, show a slight extension, with a transition to a more reddish coloration. This color gradient may indicate a variation in stellar age, metal content, or dust distribution. No prominent spiral arms or distinct features such as dust lanes are apparent. The overall morphology suggests a galaxy that has largely completed its star formation and may be approaching quiescence.
