The galaxy presents as a disk galaxy, observed at a high inclination angle, near edge-on. The disk exhibits a somewhat smooth appearance, with a subtle bulge visible. Color gradients suggest older stellar populations within the bulge and a younger population, possibly with ongoing star formation, in the disk. There is a suggestion of minor disturbances, such as slight asymmetries or distortions in the disk's morphology, potentially indicating past minor interactions. Overall, the galaxy displays characteristics of a moderately massive system with both evolved and actively star-forming regions.
