The galaxy presents as a largely smooth, centrally concentrated object with a generally elliptical morphology. A high degree of circularity is observed in its overall shape. The light profile suggests a lack of significant disk-like structure or prominent spiral arms. The color distribution appears relatively uniform across the galaxy, with a subtle shift towards redder hues in the central region and slightly bluer hues in the outer regions. There is no obvious evidence of tidal tails or other major merger signatures, although minor disturbances cannot be ruled out. Overall, the galaxy's characteristics are consistent with those of a relatively quiescent system with limited ongoing star formation.
