The galaxy presents as a spiral type, exhibiting a well-defined central bulge and a disk structure. The bulge appears prominent and relatively bright, suggesting a significant population of older stars. Faint spiral arms extend outward from the central region; they appear somewhat tightly wound. The disk is viewed at an oblique angle, though not quite edge-on, giving it a slightly elliptical appearance. There is evidence of a bar structure across the center of the bulge. The arms themselves show a mottled texture, indicative of star-forming regions interspersed with areas of lower stellar density. The overall color of the galaxy appears somewhat red, potentially indicating a relatively low rate of recent star formation throughout the galaxy.
