The observed galaxy exhibits a disturbed morphology, suggestive of ongoing or recent merger activity. Two distinct tidal tails are visible, one extending prominently from each side of the main galactic body. These tails display a bluer hue, possibly indicating regions of enhanced star formation triggered by gravitational interactions. The central region appears more concentrated, with a slightly redder color, potentially indicating an older stellar population. Overall, the galaxy appears to be a late-type spiral undergoing significant disruption. The galactic disk is difficult to observe with an edge-on view, but there appears to be at least a slight central bulge.
