The galaxy exhibits a disturbed morphology, suggestive of an ongoing or recent interaction. There is an apparent tidal tail extending outwards from the main body of the galaxy. The galaxy appears to have a disk-like structure, though it is heavily disrupted. Within the main body, there's a noticeable concentration of blue light, possibly indicating areas of active star formation. Areas of redder light can also be observed which may indicate older stellar populations or dust. Overall, the galaxy shows a complex structure, deviating significantly from a regular spiral or elliptical form. The faintness and color indices indicates a lower-mass galaxy with modest levels of star formation.
