The galaxy presents as an edge-on spiral, exhibiting a moderately elongated shape and a high degree of inclination relative to our line of sight. A prominent central bulge is visible, appearing smooth and concentrated, with a suggestion of a boxy morphology. The disk appears relatively thin and streamlined, with some evidence of dust lane obscuration along the major axis, indicating the presence of interstellar material. The disk appears somewhat asymmetrical, with the lower part of the disk displaying signs of disturbance, possibly due to tidal interactions or recent mergers. There is a smaller, rounder galaxy to the left, and there is minor disturbance in the main galaxy, suggesting possible interaction. Overall, the galaxy appears to be relatively undisturbed, with no major signs of active star formation apparent in the image.
