The galaxy appears to be a spiral galaxy viewed approximately face-on. The central bulge is prominent and exhibits a yellowish hue, suggesting an older stellar population. Spiral arms are clearly visible, emanating from the central bulge, with two arms more prominent than others. The arms appear relatively tightly wound. There is evidence of some bluer regions within the spiral arms, indicative of recent or ongoing star formation. The overall structure suggests a well-defined disk. There is a possible slight disturbance in the morphology, with some asymmetry, but it does not appear to be a major merger event.
