The galaxy presents as a lenticular or possibly spiral galaxy viewed at a high inclination, appearing as an elongated, somewhat flattened disk. A bulge is subtly visible, showing a concentration of light towards the center of the disk. The primary color is a yellowish-orange hue, suggesting an older stellar population, with some bluer regions visible, indicating regions of active star formation. No strong signs of tidal disturbance or ongoing major merger events are observed, though there may be minor irregularities in the disk structure that suggest a possible past interaction or minor merger event. The smooth, diffuse light profile suggests a relatively evolved system.
