The galaxy presents as a single dominant spheroid of concentrated light, suggesting an elliptical morphology. There is a distinct secondary object located to the left side of the dominant galaxy. The object presents as a smaller, less concentrated spheroid. There is some distortion within the primary galaxy's halo, with a slight elongation towards the secondary object. These observations suggest a possible ongoing or recent interaction between the two galaxies. The overall color profile appears to be on the redder end of the spectrum, suggesting an older stellar population with relatively low levels of ongoing star formation. The main body of the galaxy exhibits a smooth and rounded appearance, typical of early-type galaxies.
