The galaxy appears to be a relatively small, edge-on spiral galaxy. It exhibits a smooth, elongated profile with a high degree of central concentration. The central bulge is bright and slightly blue, suggesting ongoing or recent star formation. The disk component, while viewed edge-on, appears relatively thin and elongated with a hint of dust lanes visible. The overall color suggests a galaxy with a intermediate rate of star formation activity. There is no apparent tidal disturbance or evidence of a major merger event. The galaxy looks relatively isolated and unperturbed.
