The galaxy exhibits a predominantly disk-like morphology. The disk is seen at an angle, and appears elongated. Some form of weak spiral structure may be present, with bluer regions possibly indicating areas of active star formation. These regions are primarily observed at both ends of the disk. The central region is noticeably more luminous and yellowish, suggestive of an older stellar population and possibly a bulge component. The galaxy is relatively smooth in appearance, with no obvious signs of major merger activity or strong tidal disturbances.
