The galaxy presents as a multi-component system, potentially undergoing interaction or in close proximity with multiple companions. The primary structure appears somewhat irregular, exhibiting a disturbed morphology rather than a well-defined spiral or elliptical shape. Evidence of a possible tidal tail or bridge-like structure suggests gravitational interaction with a nearby object, potentially contributing to the observed distortion.

There appears to be some substructure within the galaxy, possibly indicative of star formation regions. The bluer colors may suggest the presence of younger, hotter stars within these regions. Overall, the galaxy seems to be in a dynamic state, with ongoing or recent interactions likely influencing its structure and star formation activity.
