The galaxy appears to be a disk galaxy, seen nearly edge-on. A prominent central bulge is visible, appearing elongated along the plane of the disk. The bulge exhibits a mostly smooth, but not perfectly spherical, morphology. The galactic disk shows some evidence of dust lanes or obscuring material along its length, contributing to a somewhat disturbed visual appearance. The overall color is dominated by warmer tones toward the bulge, suggesting an older stellar population, with hints of bluer hues in the outer regions of the disk, which could indicate more recent star formation. No obvious spiral arm structure is discernible from this viewing angle, but the disk displays an irregularity suggestive of minor gravitational disturbances. There is no evidence of significant ongoing mergers with other galaxies, although some tidal features or faint extensions might be present upon closer examination. The galaxy does not seem to be experiencing major bursts of star formation.
