The galaxy exhibits a disk-like morphology, with a moderate central bulge. The disk itself is not perfectly face-on, showing a slight inclination with respect to our line of sight. Diffuse spiral arm structures are discernible. The overall color suggests a galaxy that is actively forming stars, with a bluer hue indicating the presence of younger, hotter stellar populations. The disk appears relatively smooth, suggesting a degree of morphological maturity, however, some irregularities may indicate minor disturbances or recent interactions. The galaxy's shape appears elliptical.
