The galaxy presents as a relatively small, edge-on or highly inclined spiral. A distinct central bulge is visible, appearing smooth and concentrated, with a yellowish-orange hue. Fainter, bluer light extends along the galactic plane, suggesting the presence of a disk with ongoing star formation. This disk appears somewhat patchy or uneven, showing possible dust lanes or spiral arm segments. The overall shape is elongated, with a ratio of the minor to major axis under 0.8, indicating a flattened structure. There is no strong evidence of major mergers or tidal disturbances in the immediate vicinity of the galaxy.
