The galaxy presents as a relatively smooth, elliptical or lenticular structure. There is a slight elongation, deviating from a perfectly circular morphology. The galaxy exhibits a concentrated central bulge that diffuses outward, with a noticeable lack of defined spiral arms or prominent dust lanes. Color gradients suggest a population dominated by older stars, with a yellowish-red hue overall, indicating minimal ongoing star formation. The light distribution is smooth and symmetric, without major disturbances or signs of recent mergers.
