The object exhibits a flattened, disk-like morphology with a noticeable central bulge. The galactic disk presents a complex structure with what appear to be several faint spiral arm segments. These arms are not clearly defined, hinting at a flocculent or disrupted spiral structure. The galaxy displays color gradients, transitioning from a bluer hue in the outer regions of the disk to a slightly redder hue in the central bulge. There is an irregular feature possibly related to tidal disturbance or possible ongoing minor merger in the galaxy. Overall the galaxy does not seem to be a typical spiral or elliptical galaxy.
