The galaxy presents as a centrally concentrated object with a smooth, relatively featureless morphology. The overall shape appears somewhat elliptical, though precise classification is challenging given the image resolution. The light distribution suggests a dominant bulge component, with a gradual decrease in intensity towards the outer regions. The color profile is characterized by a reddish-yellow hue, indicative of an older stellar population and lower ongoing star formation. There is no clear evidence of spiral arms or prominent dust lanes. A minor disturbance or possible interaction cannot be ruled out completely, though any such features are subtle.
