The galaxy appears as a relatively smooth, elongated object. It exhibits a noticeable central bulge that is brighter and more concentrated than the surrounding disk. The light from the central bulge is yellowish, suggesting an older stellar population. The disk appears significantly thinner and exhibits a bluer hue, possibly indicative of ongoing star formation. The overall morphology suggests a galaxy that could be classified as an elliptical, with some minor features present that could indicate minor disturbances within the galaxy.
