Observed galaxy appears as a moderately bright, disk-shaped structure, with an approximate semi-major axis of 7 arcseconds. The central region exhibits a bright, concentrated core. The overall color suggests a galaxy with a moderate population of young stars, potentially undergoing active star formation. Evidence indicates that the galaxy has a disturbed morphology. There are faint tidal features apparent, with hints of asymmetry in the galactic disk. The color gradients and irregular shape suggest a possible recent or ongoing interaction or merger with another galactic object.
