This galaxy presents as a spiral galaxy with a moderate inclination. It exhibits well-defined spiral arms, predominantly displaying a two-arm structure. The winding of the spiral arms is observed to be of medium tightness. A central bulge is evident, appearing to be of moderate size. A bar structure is present, albeit weakly defined. There is no visual evidence of any significant ongoing mergers, though minor disturbances are indicated by some asymmetry in the arm structure. Star formation appears active within the spiral arms, as indicated by the blue color, while the bulge has a yellowish hue, indicating older stellar populations.
