The galaxy presents an irregular morphology, possibly indicating a recent or ongoing merger event. Two distinct, bright nuclei are apparent, each surrounded by diffuse stellar material. The overall color is bluish, suggesting the presence of relatively young, hot stars. There is no discernable spiral structure or prominent dust lanes; the galaxy is primarily amorphous in appearance. The luminosity is moderate and the star formation rate appears low, indicating a relatively quiescent system. The presence of two nuclei suggests it may be the result of the interaction between two separate galaxies. There is evidence of tidal distortions with a slight plume visible which indicates a merger is happening. The galaxy is faint, and seems to be a small dwarf galaxy.