The galaxy appears to be a spiral galaxy, although somewhat indistinct. It presents a moderate bulge at its center, with a yellow-white hue indicating an older stellar population. The disk surrounding the bulge exhibits a blueish tint, hinting at the presence of younger, hotter stars and ongoing star formation. The spiral arms are somewhat tightly wound. There are indications of at least two spiral arms. There is no clear evidence of a bar structure. There are no obvious signs of major disturbances due to mergers or interactions with other galaxies.
