The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. The light profile is dominated by a bright, yellowish core, suggesting an older stellar population. A faint blue disk is also present surrounding the bulge. The smooth appearance of the galaxy indicates it has likely undergone significant dynamical relaxation, and is in a relatively stable state, though minor disturbances could be present. There may also be a very small disk surrounding the bulge. The intermediate roundness suggests it is not a perfect sphere nor a highly elongated cigar shape. There does not seem to be a strong presence of ongoing, major star formation activity given the overall color distribution.
