The galaxy presents a clear disk structure, observed at an angle close to face-on. Prominent spiral arms extend from the central bulge, exhibiting a well-defined, two-armed morphology. These arms display a somewhat flocculent structure, with segments appearing more tightly wound towards the center and looser at the periphery. A bar structure appears to be present. The central bulge appears of moderate size relative to the disk. No signs of major mergers or significant disturbances are immediately apparent, though minor tidal features may be present. The galaxy is likely a spiral galaxy with ongoing star formation.
