The galaxy presents as an elongated, cigar-shaped system, likely viewed edge-on or at a high inclination. It exhibits a smooth, centrally concentrated bulge, with a gradual fading of luminosity towards the edges. The core appears yellowish-white, possibly indicating an older stellar population. There are hints of bluer colors on the periphery of the galactic disk, perhaps indicating regions of ongoing star formation, but this is difficult to confirm with certainty. No distinct spiral arm structures or bars are readily apparent, with any such features potentially obscured by the viewing angle. There is no obvious evidence of any recent major merger events. Minor disturbances cannot be ruled out.
