The galaxy presents as a face-on spiral, exhibiting a discernible disk structure with relatively tightly wound spiral arms. The central bulge is prominent, with a moderate size relative to the overall disk. The light distribution suggests an older stellar population dominating the bulge, indicated by the yellowish hue. The spiral arms exhibit a bluer color, implying ongoing star formation. There appears to be two dominant spiral arms. There is no evidence of a major merger. Minor disturbances could be present within the outer disk.
