The galaxy exhibits a distinct spiral morphology. Two prominent spiral arms are clearly visible, emanating from a bright central bulge. These arms appear relatively tightly wound around the bulge, indicating a potentially higher shear rate in the galactic disk. There is a strong indication of active star formation occurring within the spiral arms, as evidenced by the presence of numerous bright knots and regions of enhanced luminosity. The central bulge dominates the galaxy's overall luminosity profile, suggesting a significant concentration of older stellar populations in the galactic core. The disk component appears somewhat thinner relative to the bulge size. A slight asymmetry or disturbance is visible in the outer regions of the disk, potentially indicative of a past or ongoing minor interaction with another galaxy, but for the most part it appears to be an undisturbed system. There's a suggestion of a central bar structure, although not prominent.
