The galaxy presents a lenticular morphology, appearing mostly smooth and relatively featureless. The light distribution suggests a centrally concentrated bulge, gradually fading into the outer regions. The shape is somewhat elongated, deviating slightly from perfectly circular, but not cigar shaped. Subtle indications of minor disturbances or interactions appear as a slight irregularity in the outer halo. The color gradients appear relatively uniform, with minimal evidence of distinct star-forming regions. The overall color index suggests a population of older stars dominating the luminosity output.
