The galaxy appears as a largely featureless elliptical, exhibiting a smooth, diffuse light distribution with no discernable spiral arm structure or prominent dust lanes. The central region of the galaxy appears brighter and more concentrated, gradually fading towards the outer edges. The overall color is a warm, reddish-orange hue, suggestive of an older stellar population, with relatively little active star formation. The galaxy shows a slight degree of ellipticity, with a nearly circular shape. There is no evidence of tidal tails, strong gravitational lensing effects, or ongoing major merger activity. The morphology suggests a galaxy that has largely completed the process of hierarchical assembly, with minimal recent interactions.
