The galaxy presents as a complex, merging system. There are multiple distinct luminous components visible. One is a seemingly older stellar population, exhibiting a yellowish hue, potentially indicating a population of evolved stars. Another component is much bluer, suggestive of active star formation occurring within that region. The third component has a red hue, that can either be interpreted as a dusty region or a region with redshifted emissions.

There are some apparent tidal disturbances, suggesting an ongoing or recent gravitational interaction between the components. The overall shape deviates significantly from a standard elliptical or spiral morphology, further supporting the merging scenario. The spatial extent is not particularly large, seemingly compact. The colors are indicative of ongoing star formation.
