The galaxy appears to be an elliptical galaxy, characterized by a smooth, centrally concentrated light distribution. The light profile exhibits a high degree of radial symmetry, and the isophotes appear generally rounded, although not perfectly circular. There is no obvious spiral arm structure or dust lane indicative of a disk component. The galaxy appears to be dominated by older stellar populations, as evidenced by the yellowish-red hue which dominates the central regions. The overall color suggests relatively low levels of ongoing star formation, consistent with a population of older, redder stars. There is no evidence of a strong tidal disturbance or ongoing merger activity, although minor asymmetries cannot be ruled out.
