The galaxy presents as a flattened, cigar-shaped morphology, indicative of an edge-on spiral or lenticular galaxy. It exhibits a noticeable central bulge that appears yellowish-white in color, possibly suggesting an older stellar population. A disk component is also visible, displaying a bluer hue, hinting at more recent star formation activity. The galaxy appears relatively smooth with a somewhat disturbed morphology. There is minimal evidence of a major merger but a minor disturbance might be occuring. The galaxy does not appear to be a pure elliptical, exhibiting some degree of structure within its disk.
