The galaxy presents as a diffuse, yellowish-white elliptical system. There is evidence of some irregular structure with fainter, blueish arms or streams emanating from the central region. The core of the galaxy appears quite smooth and centrally concentrated, with a gradual decrease in luminosity outward. There is a slight elongation, suggesting it is not perfectly spherical. It exhibits faint hints of a disk. There are also several other smaller, likely background galaxies and bright knots of star formation in close proximity, that may be interacting with the central galaxy. Some of these knots show bluer colors, possibly indicating recent star formation, while others appear redder and potentially older. There is evidence of a possible merging event.
