The galaxy presents a morphology exhibiting both smooth and featured characteristics. The central region displays a relatively smooth profile, transitioning outward into a disk-like structure with observable features. The color distribution suggests variations in stellar populations. A dominant green hue is visible throughout, possibly indicating the presence of ionized gas. The presence of redder components implies the presence of older stellar populations or dust obscuration within certain regions. The galaxy may be currently undergoing, or have undergone, some form of minor interaction. There are some signs of disturbance in the shape. However, a more comprehensive analysis involving spectroscopic data would be necessary to confirm these hypotheses.
