This galaxy appears to be a spiral galaxy, possibly viewed edge-on or at a very high inclination. A central bulge is visible, appearing relatively smooth and elongated, with a slightly brighter concentration toward the geometric center. Fainter, bluer light extends outwards from the bulge, suggesting the presence of a disk. The disk appears somewhat asymmetrical, with noticeable disturbances or irregularities in its structure. The overall color suggests the presence of ongoing star formation, particularly within the disk. Evidence of possible tidal interactions or minor mergers is present, indicated by the distortions and asymmetries observed in the disk morphology. The galaxy displays an apparent size of approximately 8 arcseconds.
