This galaxy exhibits a clear disk structure, viewed at an oblique angle, but with significant disruption evident throughout the galactic body. A prominent central bar feature is present, elongated along the major axis of the disk and displaying a yellowish hue, suggestive of an older stellar population. The spiral arms are readily identifiable, though somewhat irregular and distorted. One of the arms appear tightly wound closest to the center of the galaxy, while the other arm flares out, indicating an asymmetry in its structure. The arms appear to be the dominant structure compared to the bulge, which is small and unassuming. Blueish regions of star formation can be seen in both of the spiral arms. Indications of a potential tidal interaction or ongoing merger event are present, with a lopsided morphology and a large distorted feature present around the galaxy. These features suggest gravitational disturbances affecting the galactic structure.
