The galaxy presents as a disk galaxy observed at a near edge-on inclination. A prominent dust lane bisects the galaxy, obscuring a substantial portion of the galactic plane. The bulge appears centrally located and exhibits a yellowish hue, suggesting an older stellar population. The disk component displays a bluer color, indicative of ongoing star formation. The overall morphology appears relatively undisturbed, though some minor irregularities in the disk structure are present, potentially indicative of minor interactions or internal dynamics. It appears to be undergoing star formation at a moderate rate. The size is moderate for a disk galaxy.
