The galaxy presents as a singular, moderately bright object, approximately elliptical in shape. There is evidence of a bulge, which appears bright and concentrated, with a distinctly blue-white color indicative of a population of hotter, younger stars. The outer regions of the galaxy exhibit a green hue. A smaller red area is visible near the bottom edge of the galaxy. There is also an extended fainter area near the bottom of the galaxy with a green hue, suggesting some form of galactic disturbance or interaction. Overall, there does not appear to be a dominant spiral structure or a particularly smooth, featureless appearance. 
