This galaxy presents as a spiral type with well-defined spiral arms. There's a discernible central bulge region appearing with a yellowish hue, suggesting an older stellar population residing there. The arms exhibit a bluer color, indicative of ongoing star formation activity. The spiral structure appears relatively tightly wound. The galaxy appears relatively undisturbed. The disk of the galaxy appears tilted relative to our line of sight, allowing for a clear view of the spiral arms. There may be a weak bar-like structure present in the center.
