The galaxy presents as a spiral galaxy, exhibiting a prominent disk structure with observable spiral arms. The galaxy is not perfectly face-on but is observed at a slight angle, which allows for the identification of spiral features. The arms appear relatively tightly wound around a central bulge region. The central bulge appears moderately sized compared to the overall disk, displaying a yellowish hue, indicative of an older stellar population. The spiral arms show a bluer tint, suggesting ongoing star formation activity. There may be two main spiral arms, though some arms may be indistinct. It is possible that the galaxy is currently undergoing or has recently experienced a minor disturbance, given some irregularity in its spiral arm structure. Overall, the galaxy exhibits characteristics of a barred spiral. The colours shown suggest ongoing star formation.
