The galaxy appears to be a disk galaxy viewed edge-on. A prominent, relatively bright bulge is visible, appearing more rounded than boxy. There is evidence of some dust lane obscuration along the galactic plane, though subtle. The disk itself seems relatively smooth, with the suggestion of spiral arm structure hinted at through slight variations in color and brightness, but they are not well-defined. The galaxy exhibits a color gradient, with the bulge exhibiting a yellow to reddish hue, possibly indicating an older stellar population, while the outer disk appears bluer. The overall morphology suggests a relatively undisturbed system, with no obvious signs of a major ongoing merger, though a minor disturbance cannot be entirely ruled out. The light distribution suggests a galaxy with a relatively high stellar mass and moderate star formation activity.
