The galaxy presents a relatively smooth, elliptical morphology. Its core appears bright and concentrated, exhibiting a yellowish hue indicative of an older stellar population. The outer regions of the galaxy fade gradually into the background sky, suggesting a lack of distinct spiral arms or prominent star-forming regions. There is a slight elongation visible, deviating from a perfectly circular shape. Faint blue tinges are observed within the halo, suggesting there may be a small amount of recent star formation. Overall, the galaxy appears largely undisturbed.
