The galaxy appears as a moderately bright, elongated structure with a slight bulge, potentially an early-type spiral or a lenticular galaxy. It is viewed at a high inclination. The central region exhibits a concentration of light, suggesting the presence of a galactic nucleus. The light is redder compared to the edges. This is likely due to older stellar populations. There appears to be evidence of a slight disturbance. It could be the result of a minor interaction or merger. There is a hint of asymmetry, more apparent on the left side.
