The galaxy presents as a relatively smooth, concentrated object, appearing mostly round in shape. A slight elongation is possibly present, though the general form is nearly circular. A noticeable color gradient is observable, with a central, bright region exhibiting a yellowish to almost white hue, suggesting the presence of an older stellar population. The outer regions display a subtle redder tint indicating possibly lower rates of star formation. Overall the galaxy shows no signs of major disturbances or merger events. The morphology is consistent with an elliptical galaxy with an estimated size around 3.5 kpc.
