The galaxy exhibits a morphology consistent with an ongoing or recent merger event. It presents as two distinct nuclei or regions of high stellar density. The upper nucleus displays a yellowish-white hue suggesting an older stellar population, with potentially lower ongoing star formation. The lower nucleus appears slightly more diffuse and exhibits a warmer, reddish-orange color, which might indicate more recent or ongoing star formation activity as well as significant dust presence. There's a faint tidal feature or bridge of material connecting the two nuclei, visible as a faint, nebulous extension. Overall, the galaxy has a disturbed, irregular appearance indicative of gravitational interaction. The system appears relatively compact, with the entire interacting system spanning an estimated diameter of about 2.5 kpc. The system displays a relatively smooth light distribution overall.