The galaxy presents as a spiral system with a notable central bulge. The bulge region appears relatively smooth and featureless, exhibiting a bright, concentrated luminosity. Surrounding the bulge, spiral arms are discernible, although somewhat tightly wound. The arms appear to be primarily composed of older stellar populations, based on their color. There are regions of bluer color, indicating recent star formation within the arms, though these are not highly pronounced. The galaxy appears to have moderate internal structure. The overall shape of the galaxy approximates a flattened disk viewed at an oblique angle. There are no obvious signs of a major ongoing merger event, although some minor asymmetries or disturbances in the spiral arms suggest possible past interactions or internal dynamical processes. The galaxy appears relatively isolated in the image, with no nearby interacting galaxies of comparable size.
