The galaxy presents as a face-on spiral, with a bright central bulge exhibiting a yellowish hue. Faint spiral arms extend outwards from the central region, appearing somewhat tightly wound. These arms display a blueish color, suggesting the presence of relatively young, hot stars. The disk component dominates the overall structure, obscuring a significant portion of the central bulge. There appears to be no strong bar feature across the galaxy's center. The galaxy does not show signs of a major merger event, but subtle irregularities in the spiral arms could indicate minor gravitational interactions or disturbances. Overall, the galaxy appears relatively well-defined with a moderate amount of light emitted.
