This galaxy presents as a spiral, viewed at a significant angle, though not perfectly edge-on. A prominent disk structure is evident, exhibiting a moderate inclination relative to our line of sight. There are indications of spiral arm morphology, though the arms appear somewhat flocculent and not tightly wound. Color gradients suggest active star formation regions, particularly in the outer regions of the disk. The galaxy displays a noticeable central bulge of moderate size. Based on the irregular shape and the overall color profile, this galaxy may be undergoing some form of interaction or disturbance. There appears to be faint tidal features present that support this hypothesis. It is a relatively massive object, and is actively forming stars, but at a rate that is slowly decreasing. A bar structure cannot be definitively discerned from this image.
