The object presents as a spiral galaxy, displaying a prominent disk-like structure. The galactic core exhibits a concentrated, bright, yellow-orange hue, suggesting an older stellar population is dominant. Spiral arms are visible, though somewhat tightly wound. Indications of ongoing star formation, marked by regions of blue-ish light, are discernible within the arms. Some regions of disruption can be observed. The primary galaxy also seems to be interacting or merging with a smaller companion galaxy, given their proximity and distorted shapes. The spiral arms are not evenly distributed, suggesting gravitational interactions.
