The galaxy exhibits a complex morphology, displaying characteristics of both a smooth and a featured system. A significant fraction of its light is concentrated in a central, relatively smooth component. This area presents a diffuse, rounded appearance, suggesting an older stellar population or a bulge.

Surrounding the smoother central region is a more prominent, disk-like component, discernible by the presence of clumpy features and regions of star formation. These are indicated by areas with strong blue emission. The galaxy shows signs of minor disturbances, indicated by subtle asymmetries.

The galaxy appears relatively isolated, with no indications of a major merger. Its color suggests ongoing star formation within the disk. The overall appearance suggests a spiral or irregular galaxy undergoing minor interactions or internal dynamical processes.
