The target galaxy presents a complex morphology, appearing to be undergoing a significant merger event. The primary body exhibits a distorted spiral structure, characterized by prominent, albeit disrupted, spiral arms. These arms display a medium to loose winding pattern. Two primary arms are discernable with additional arm fragments.

Evidence suggests the presence of a weak bar structure within the central region. The central bulge is of moderate size relative to the disk. There appears to be a secondary galactic component in close proximity to the primary galaxy, most likely involved in the merger. The color gradients suggest active star formation regions concentrated within the spiral arms. This galaxy shows a blue-white hue, with regions of light yellow.