The galaxy presents as a thin, elongated disk oriented nearly edge-on relative to our line of sight. A central bulge is visible, appearing somewhat rounded. Dust lanes are likely obscuring a portion of the galactic plane, causing a slight dimming and color variation along the visible length. The galaxy appears relatively undisturbed, showing no major signs of ongoing or recent merger activity. Star formation is likely occurring within the disk. The galaxy has noticeable spiral arms.