The observed galaxy appears to be an elongated spiral, viewed at an oblique angle. One can observe an inner bulge which is bright and compact, which emits mainly redder light.  Some of the fainter and bluer regions are likely in the arms of the galaxy. It exhibits asymmetrical features, with a slight curvature, which is more apparent on one side of the bulge. There is some possible disturbance in the outer regions, possibly from a past merger or interaction with another galaxy. The galaxy appears to be relatively compact in size. The color gradient suggests a relatively active star formation rate, particularly in the bluer regions.
