The galaxy presents as a smooth, centrally concentrated object, exhibiting a generally elliptical morphology. Its overall color is yellowish-white, with a slight color gradient towards the center, indicating a concentration of older stellar populations. Faint, reddish extensions are visible, potentially indicative of tidal features or ongoing minor interactions. No prominent spiral arm structure or dust lanes are discernible, suggesting an evolved system with a relatively quiescent star formation rate. A slight elongation is observed along one axis, but the overall shape remains largely consistent with an elliptical classification. There is no evidence of a major ongoing merger.
