The galaxy presents a somewhat face-on orientation, exhibiting a disk-like morphology. Spiral arm structures are discernible, loosely wound and extending from the central region. The central bulge appears relatively small and indistinct compared to the overall disk size. Patches of blue light are distributed throughout the spiral arms, possibly indicating regions of active star formation. Dust lanes appear subtly interspersed within the spiral arms. The disk appears slightly inclined, with a position angle of approximately 105 degrees, and an axial ratio suggesting it is not perfectly circular but somewhat elongated. The light distribution follows a smooth profile, generally consistent with the disk structure. Fainter outer regions extend beyond the main body of the galaxy. There is no strong evidence of a prominent bar structure.
