The galaxy presents as a somewhat distorted spiral, with an apparent central bulge and extended arms or tidal tails. The galaxy is oriented approximately diagonally in the frame.

The central region exhibits a yellowish-orange hue, possibly indicating an older stellar population. The outer regions of the galaxy display a bluer color, consistent with ongoing or recent star formation activity. Patches of blue are visible in the extended structures, suggesting areas of active star birth.

The morphology suggests possible interaction or a past merger event. The arms appear diffuse and uneven. The overall structure deviates from a grand design spiral and could be the result of gravitational interaction with another galaxy, though no obvious companion is visible in the image.

The galaxy appears moderately luminous, with a detectable extent in the image. Its redshift indicates that this object is at a considerable cosmological distance.
