The galaxy presents a largely smooth morphology, with a slight overall ellipticity. The central region exhibits a strong concentration of light, suggesting a prominent galactic nucleus. A faint, diffuse disk-like structure appears to extend outwards from the central bulge. There is evidence of possible tidal disturbances or interactions, indicated by subtle asymmetries or faint plumes extending from the main body of the galaxy. The galaxy displays a color gradient, with the central regions appearing more blue, possibly indicative of ongoing or recent star formation, while the outer regions are redder, suggesting an older stellar population. The estimated effective radius suggests this is a moderate-sized galaxy. Signs point to this being a galaxy currently undergoing a merger.
