The galaxy presents as a largely smooth, elliptical-like structure. It exhibits a concentrated central bulge, with the light appearing more intense towards the core. The overall color profile suggests a population of older stars, leaning towards redder hues, but it also has components that show relatively strong emission at shorter wavelengths. It appears quite regular in shape, with no obvious signs of ongoing major mergers or significant tidal disturbances. The overall structure appears well-defined and relatively undisturbed. The faintness of outer reaches suggests it isn't particularly active regarding star formation.
