The galaxy presents a largely smooth and centrally concentrated morphology. It appears elliptical in shape, exhibiting a moderate degree of roundness, with no obvious spiral arm structure or distinct features. The color profile suggests a dominant older stellar population, as indicated by the reddish-yellow hue of the galaxy. There is no evidence of active galactic nuclei or significant dust lanes. Given the lack of discernible tidal features or other morphological distortions, there's no indication of a recent major merger event. Faint extensions of the galaxy are subtle, but may suggest minor interactions.
