The galaxy presents as a centrally concentrated, elliptical morphology with an apparent smooth structure. The light profile suggests a high degree of radial symmetry. There is a color gradient; the central region is primarily a yellow-white hue, indicating a high population of older stars. The outer regions exhibit a bluer color profile suggesting a weak presence of younger stars. The shape is elongated, but not exceptionally so, appearing more "in-between" than overtly cigar-shaped. No strong signs of tidal disturbances or merging events are clearly visible, but very minor disturbances cannot be ruled out based on this image alone.
