The galaxy presents as a moderately luminous, elongated object. Its overall morphology suggests it is likely a disk galaxy seen at an oblique angle. There is a central bulge, characterized by a yellowish-white hue. The disk appears to be primarily smooth. There are no readily apparent dust lanes. Evidence for star formation is present, as suggested by the localized presence of blue-green regions in the disk. There appears to be no evidence of a major merger event and its disk appears to be mostly undisturbed.
