The galaxy presents a relatively smooth and featureless morphology. It appears somewhat elliptical in shape, though not perfectly round, with a slight elongation. The central region exhibits a bright concentration of light. There is evidence of a color gradient within the galaxy. The core regions exhibits light in the blue portion of the spectrum, indicating ongoing or recent star formation. The lack of prominent spiral arms or dust lanes further suggests a more evolved system with a relatively low star formation rate. The general appearance suggests a late-type spiral galaxy or an early-type elliptical galaxy. 
