The galaxy presents a disk-like morphology viewed at an oblique angle. The central bulge appears relatively small and concentrated, exhibiting a yellowish-white color indicative of an older stellar population. Prominent spiral arms extend outwards from the bulge, displaying a bluish hue suggesting the presence of younger, hotter stars and ongoing star formation. The spiral arms exhibit a relatively tight winding, with a moderate degree of fragmentation and patchy regions of star formation. Dust lanes are subtly visible within the spiral arms, particularly on the near side of the galaxy, obscuring some of the starlight. The overall color of the disk is a mixture of blue and white, with the outer regions appearing fainter and more diffuse. The galaxy appears relatively isolated, with no obvious signs of tidal distortion or interaction with neighboring galaxies. The galaxy appears to be an intermediate spiral type, showcasing features of both Sa and Sb galaxies.