The galaxy presents as a flattened, disk-like structure, viewed nearly edge-on. A prominent central bulge is observed, exhibiting a concentrated, bright, yellowish-orange hue, suggesting an older stellar population and relatively low star formation activity in the nuclear region. The galactic disk appears thin, with a faint and diffuse blueish-white color towards the outer edges, indicative of younger stars. There is no clear evidence of spiral arm structure. Some patchy irregularities are present within the disk. Overall, the galaxy appears relatively undisturbed, showing no signs of a major merger event.
