The galaxy exhibits a flattened, elliptical morphology. A prominent central bulge is observed, surrounded by a disk-like structure. Faint spiral arm features appear to originate from the bulge. There is a subtle asymmetry in the distribution of light within the disk. Color gradients are visible, with the central bulge exhibiting bluer hues compared to the outer regions of the disk, indicating a difference in stellar populations. Dust lanes are not apparent in the image. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or nearby companions.
