The galaxy presents a disk-like morphology, viewed at an angle that suggests it is not precisely edge-on. Prominent spiral arm structures are visible, though somewhat diffuse, indicating ongoing star formation. These arms emanate from a central bulge region, which appears to be of moderate size relative to the galactic disk. The disk exhibits a bluish tint, consistent with a population of young, hot stars. There is no evidence of a strong central bar structure. The overall appearance suggests a relatively undisturbed system, with no obvious signs of a major merger event currently underway.
