The galaxy appears as a moderately sized, relatively face-on spiral, exhibiting a subtle disk-like morphology. The central bulge region displays a smooth, concentrated distribution of light, suggesting an older stellar population. Faint spiral arms extend outwards, but are not sharply defined. The color gradient suggests ongoing star formation in the disk, but not at an exceptional rate. The overall light distribution is smooth, yet with a slight degree of irregularity. There are no prominent signs of a major ongoing merger, although subtle tidal features or minor disturbances cannot be ruled out. The galaxy seems to be neither perfectly circular nor highly elongated.
