The galaxy appears to be a spiral galaxy, oriented approximately edge-on to our line of sight. There is evidence of a central bulge, although it is not particularly prominent. A faint, extended disk is visible, exhibiting some signs of disturbance or asymmetry. The disk shows subtle variations in surface brightness, possibly indicating regions of differing stellar density or dust obscuration. The overall color is somewhat blueish, hinting at the presence of younger stars and ongoing star formation, though it appears to be occurring at a low rate.
