The galaxy presents as a barred spiral with a prominent central bulge. The bulge appears yellowish-white, suggesting an older stellar population and potentially a supermassive black hole at its center. The disk is oriented at a moderate inclination, revealing some spiral arm structure. These arms exhibit a clumpy morphology, hinting at active star formation regions. The overall color of the disk is bluer compared to the bulge, implying the presence of younger, hotter stars. Faint dust lanes can be inferred along the spiral arms, contributing to the observed irregularities in brightness. The galaxy has an apparent elliptical shape due to its inclination.
