The galaxy presents as an edge-on spiral system. A prominent central bulge appears yellowish-orange, suggesting an older stellar population. Fainter bluish-white light is present near the edges of the disk, likely indicating recent or ongoing star formation within the spiral arms. The disk exhibits a high degree of flattening, and it is difficult to determine the presence of a central dust lane, but a slight obscuration can be seen at the center of the disk. The bulge shows a slightly boxy shape. No signs of major mergers or strong tidal disturbances are visible. The galaxy appears relatively isolated with no close companions.
