The galaxy appears to be undergoing a significant merger event. There are at least two distinct nuclei visible, with evidence of tidal tails or distorted arms extending from the main bodies. The overall morphology is highly disturbed, exhibiting irregular shapes and diffuse regions.

The color distribution suggests varying stellar populations, with a central concentration of older, redder stars evident in the lower nucleus. Patches of bluer light are visible, particularly in the upper nucleus, indicating regions of ongoing or recent star formation. The luminosity suggests this is a moderately massive galaxy. Based on the disturbed morphology, the rate of star formation is likely elevated due to the interaction. The general shape is relatively compact, appearing neither highly elliptical nor a well-defined spiral. The presence of multiple components and the strong interactions suggest that any pre-existing disk structure has been significantly disrupted.
