The galaxy presents as an elongated, disk-like structure seen nearly edge-on. A prominent central bulge is visible, appearing relatively smooth and concentrated. The disk component exhibits a mottled texture, hinting at some substructure, possibly spiral arms or dust lanes, but the high inclination makes these features difficult to resolve. Overall the galaxy appears smooth, but there seems to be a small amount of galactic disturbance. The galaxy's light profile suggests that it is a relatively small, low-mass galaxy. There appears to be a low rate of star formation.
