The galaxy presents as an irregular morphology with evidence of tidal disturbance. Multiple luminous knots are apparent within the main body of the galaxy, suggesting active regions of star formation. The overall color is bluish, indicative of a relatively young stellar population. The galaxy appears to be undergoing a major merger with another galaxy or has been affected by a significant interaction in the recent past. There are possible remnants of tidal tails extending from the main galactic body, though these are faint and difficult to ascertain with certainty.
