The galaxy presents as a relatively smooth, disk-like structure. Its overall shape is somewhat elongated but largely featureless, indicating it's likely an elliptical galaxy. There is a central bulge that appears brighter and more concentrated than the outer regions of the galaxy. The galaxy exhibits a redder hue, suggesting an older stellar population with lower rates of current star formation. There may be a minor disturbance in structure, but no major mergers are apparent in the image. It would appear to be a mature and stable galaxy. 
