The galaxy presents as a diffuse, somewhat amorphous structure. There is a central concentration of light, however, the overall distribution appears uneven. A blue hue is seen throughout the galaxy, indicating the presence of relatively young, hot stars and ongoing star formation. Evidence of disruption suggests a possible past or ongoing interaction. Specifically, the structure seems asymmetric, possibly exhibiting tidal features, consistent with a disturbed morphology. There are no clear spiral arm structures, and no significant dust lanes are apparent in this image. The galaxy does not present with a regular, defined structure, and appears to be actively interacting with another body.
