This galaxy appears to be a relatively bright, moderately sized system. The overall morphology suggests a primarily smooth structure. There is a distinct central bulge with a high degree of circularity. Evidence of a disk component is present, though it is not sharply defined. There are asymmetries within the disk suggesting possible gravitational interactions. The galaxy exhibits a green hue, which could indicate star formation. The galaxy may be undergoing or has recently undergone a minor merging event.