The galaxy presents as a spiral type, exhibiting distinct, well-defined spiral arms. The arms appear tightly wound near the core, transitioning to a more moderately wound structure as they extend outward. A bulge is present, exhibiting a moderate size relative to the disk. Evidence suggests this galaxy may be interacting with another galaxy, showing subtle disturbances in morphology, but shows no merging. There appears to be a potential bar feature. The disk component is the dominant feature of the galaxy, its spiral structure more pronounced than the bulge. The overall color profile is a general spiral.
