The galaxy presents a smooth, elliptical morphology. It is moderately elongated, exhibiting an axis ratio suggesting it is somewhere between a spherical and cigar shape. The light distribution is centrally concentrated, with a bright core that diffuses outwards. There is a color gradient, with the central region appearing whiter, potentially indicating an older stellar population. Fainter, bluer hues are observed in the outer regions, possibly suggesting some ongoing star formation, though the overall smoothness indicates this is not a dominant process. There are no apparent signs of significant disturbances such as tidal tails or strong asymmetries to indicate a recent major merger event.
