This galaxy presents a distinct spiral structure, exhibiting prominent, though somewhat disrupted, spiral arms. The arms appear patchy, with visible clumping of stars and gas. A central bulge is evident, appearing moderately sized and slightly elongated. There is suggestion of a bar-like feature bisecting the bulge, potentially a weak or nascent bar structure. Overall, the galaxy displays a disk-dominated morphology, with the spiral arms contributing significantly to its luminosity. The disk does not appear to be perfectly face-on; it presents with a slight inclination to the line of sight. There is no obvious evidence of a major ongoing merger, although minor tidal disturbances cannot be ruled out based on this image. Color gradients suggest active star formation regions within the arms.
