The galaxy presents as a flattened, disk-like structure, viewed at a significant angle to its plane. The central region exhibits a concentrated, bright, yellowish-orange hue, likely indicating a bulge dominated by older stellar populations. Moving outward from the center, the disk appears less structured. Some faint blue regions are visible within the disk, suggesting areas of more recent star formation. Overall, the galaxy appears relatively undisturbed with no obvious signs of major mergers or tidal interactions. The galaxy displays characteristics of a spiral galaxy, however the spiral arms are not well defined.
