The galaxy presents a spiral morphology, characterized by a noticeable disk structure with prominent spiral arms. These arms appear somewhat tightly wound closer to the galactic center, and gradually loosen further away. The presence of at least two distinct spiral arms is suggested by the observed features, with some areas displaying more diffuse structure. The core exhibits a strong central bulge with a concentrated brightness. Overall the galaxy appears relatively undisturbed, with no major signs of tidal interactions or ongoing merger events visible. A faint bar-like structure seems to be present within the disk. The disk orientation appears to be close to face-on, with the arms extending outwards in a pinwheel shape.
