The galaxy presents as a late-type spiral, viewed edge-on. There is a central bulge, displaying a relatively smooth texture with a concentrated intensity, indicating a possible evolved stellar population. The disk component is visible as a faint, elongated structure extending outwards from the bulge. There are hints of spiral arm structures within the disk, showing slight color variations with bluer regions which hint at ongoing star formation. The overall form of the galaxy appears relatively undisturbed, suggesting that it has likely not undergone any recent major mergers. The mass of the galaxy is relatively high, meaning this is most likely a spiral galaxy.
