The galaxy presents as an elongated, flattened spheroid, suggesting an elliptical morphology. The central region exhibits a higher surface brightness, indicating a concentration of stars and potentially a supermassive black hole. The light distribution appears smooth and diffuse, lacking prominent spiral arms or distinct features. The overall color is relatively uniform, tending toward a pale blue hue. There is no evidence of significant dust lanes or ongoing major star formation regions within the galaxy. The galaxy's profile is more elongated than it is round, indicating a high ellipticity.
