The galaxy presents an elliptical morphology, appearing largely smooth and centrally concentrated. A prominent bulge dominates the structure, exhibiting a yellowish-orange hue indicative of an older stellar population. There is some indication of a weak disk surrounding the bulge, but no spiral arms or distinct features are discernible. The overall color suggests moderate star formation activity. The galaxy shows no strong signs of ongoing merger events or major disturbances. The shape appears to be fairly round. 
