The galaxy appears to be a disk galaxy, seen at a high inclination. There is a bulge or central concentration that is bright in the center, which could be caused by higher star density, or possible Active Galactic Nucleus. The colors range from red to green, though the galaxy appears blue overall. The colors suggest variations in stellar populations and star formation activity within the disk. Faint spiral arm structures may exist, but are not easily distinguished. The disk shows some irregularities in surface brightness, suggesting possible interactions with another galaxy, or recent merger activity.
