The galaxy presents a clear disk-like morphology, viewed nearly edge-on. A central bulge, appearing yellowish, is prominent, suggesting an older stellar population concentrated in the core. The disk itself exhibits a bluish hue, indicative of ongoing star formation and the presence of younger, hotter stars. Evidence of some spiral structure is present within the disk, though it appears somewhat irregular and disturbed. The dust lanes are subtle, but present in the disk, providing contrast. Overall, the galaxy displays features that are consistent with a spiral galaxy, however the presence of disturbances suggests a possible interaction or merger event in its past.
