The galaxy presents as a disk galaxy, observed at a moderate inclination. It is approximately 8 kiloparsecs in radius. The central bulge appears prominent and exhibits a yellow-orange hue, potentially indicative of an older stellar population. The disk displays bluer arms, suggesting ongoing star formation. The overall morphology appears relatively undisturbed, with no obvious signs of major mergers, though there is some asymmetry present. The galaxy appears to be moderately massive with ongoing star formation.
