The object presents as an elongated, disk-like structure, oriented horizontally in the image. The central region exhibits a high surface brightness, appearing almost stellar in nature, and is noticeably bluer than the outer regions.

Moving outward from the bright center, a more extended, less luminous disk is observed. This disk shows some color variation, with the left side appearing somewhat greener and the right side showing hints of redder hues. The edges of the disk are not sharply defined, blurring into the background sky.

There are some irregularities or disturbances visible within the disk. Overall, the galaxy appears to be undergoing some form of interaction or internal process that is disturbing its morphology.
