The galaxy appears as a somewhat elongated, diffuse object. A central bulge is visible with a brighter, more concentrated core region. The overall color of the galaxy is predominantly bluish-white, suggesting a significant population of young, hot stars, particularly within the central region and areas of the disk. The disk component is weakly defined, possibly indicating a lenticular or early-type spiral morphology. There appears to be a faint, asymmetric extension or tidal feature on one side of the galaxy, potentially suggesting minor gravitational interaction. The overall smoothness of the galaxy indicates a degree of morphological evolution, with a generally well-mixed stellar population.
