The galaxy presents as a single, luminous object appearing approximately round in shape, with a slightly irregular morphology. The light distribution is uneven, suggesting a non-uniform stellar population or dust obscuration within the galaxy. There appears to be a complex internal structure, possibly indicative of an ongoing or recent merger event. A possible tidal tail or bridge-like feature suggests an interaction or disturbance. Overall, the galaxy exhibits signs of significant activity, potentially driven by mergers or other dynamic processes.
