The galaxy exhibits a complex morphology, suggesting ongoing or recent interactions. Its overall structure appears disk-like but with significant distortions. The central region displays a prominent, elongated bulge, characterized by a yellowish-orange hue, indicating a population of older stars. Faint spiral arm structures are visible, though they are disrupted and asymmetrical. A significant portion of the galactic disk appears distorted, possibly indicative of tidal forces. Patches of bluer light, indicative of younger stellar populations and star formation, are scattered throughout the disk, particularly in the regions of apparent disturbance. A large, diffuse halo surrounds the central structure, showing an irregular shape. There is no singular distinct core, further suggesting it could be the result of an interaction or merger.
