The galaxy presents as an elongated, disk-like structure oriented nearly edge-on relative to our line of sight. A central bulge, exhibiting a smooth, rounded morphology, dominates the luminosity. Fainter, diffuse light extends outward from the bulge along the plane of the disk, tracing the distribution of stellar populations and dust. The overall color suggests a redder stellar population, possibly indicative of an older population of stars with a low star formation rate. There is a slight blue region visible which likely indicated a younger population. The relative lack of clearly defined spiral arms suggests a smooth stellar distribution within the disk, typical of galaxies that are at an advanced evolutionary state. A lack of any signs of tidal features or disturbances suggests that there has not been a recent major merger event.
