The galaxy presents as a relatively smooth, rounded object with a concentrated central bulge. There is a discernible, though faint, disk-like structure surrounding the bulge, giving it a slightly elongated appearance. The color gradient transitions from a yellowish core to a greenish outer region, potentially indicating differing stellar populations or dust distribution. There are no obvious signs of spiral arms or bar features. The galaxy appears relatively undisturbed, with no major distortions or tidal tails suggestive of recent major mergers. A slight asymmetry in the disk's outer edges cannot be ruled out.
