The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge. The light distribution appears relatively uniform, lacking prominent spiral arms or distinct substructures. The galaxy's color profile indicates a prevalence of older stellar populations, which likely contribute to its overall reddish hue. There is evidence of minimal ongoing star formation. The shape exhibits an approximate circularity, deviating only slightly from a perfect sphere. There is no visual indication of major tidal disturbances or ongoing merging activity, though there are indications of minor disturbances.
