The galaxy presents as a spiral type, exhibiting well-defined, loosely wound spiral arms. The arm structure appears two-armed. The central bulge is small and unobtrusive with a moderate concentration of light, transitioning smoothly into the disk. There is no apparent bar structure. Star formation appears widespread across the disk, particularly along the spiral arms. Faint disturbances are visible, with no indication of a major merging event. Overall, the galaxy exhibits characteristics of a relatively undisturbed spiral galaxy with ongoing star formation.
