The galaxy presents a distinct disk-like structure, viewed at a moderate inclination angle. Spiral arm features are apparent, though not sharply defined, appearing somewhat flocculent in nature. A central bulge is observable, with a luminosity that suggests it is of moderate size relative to the overall disk. The color distribution indicates active star formation regions within the disk, contributing to the overall blue tint. There may be a bar feature present. There is no significant evidence of major interaction or merging events.
