The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology with a high degree of roundness, showing minimal signs of a disk-like structure. There is no significant evidence of ongoing mergers or major disturbances in its overall structure. The color suggests the presence of an older stellar population. While there is a minimal amount of active star formation occurring, with a low star formation rate, it seems to be a fairly mature galaxy. 
