The galaxy presents as a well-defined spiral structure, exhibiting a classic morphology. Multiple spiral arms are visible, appearing tightly wound around a central bulge. The bulge itself presents a yellowish hue, possibly indicating an older stellar population. The spiral arms display a bluer color, suggestive of ongoing star formation. The overall disk appears relatively undisturbed, with no obvious signs of major mergers or interactions. There may be a hint of a weak bar structure in the central region. The majority of the galaxy appears to lie flat against the plane of observation, with minimal signs of inclination. There appear to be multiple star-forming regions, or areas of concentrated hot, blue stars, visible along the arms. The galaxy demonstrates a notable central luminosity concentration, indicating a prominent bulge, surrounded by a more diffuse disk.
