The galaxy presents as a disk-shaped structure with a noticeable bulge. The luminosity is concentrated toward the central region, gradually decreasing outwards. The bulge region appears yellowish-white. The disk is observed nearly edge-on, with some obscuration likely due to dust lanes or patchy distribution of dust. A slight asymmetry is noticeable in the disk's outer regions. There is evidence of star formation, particularly in the outer regions of the disk.
