The galaxy presents as an edge-on spiral, exhibiting a distinct flattened disk structure. A prominent central bulge is observed, with a rounded morphology. There are hints of possible dust lanes obscuring the galactic plane. The galaxy exhibits a yellow-red hue, possibly indicating an older stellar population or significant dust extinction. The absence of well-defined spiral arm structures suggests it might be a relatively smooth disk. No signs of tidal tails or major distortions are immediately apparent, implying that this galaxy is relatively undisturbed in its local environment, however, minor disturbances cannot be ruled out. There is also a slight irregularity in the galactic disk.
