The galaxy presents as a relatively smooth, elliptical structure, with no immediately apparent spiral arm features. Its overall shape is elongated, approximately 4.2 kpc in diameter. The light distribution is concentrated towards the center, suggesting a dense nucleus. The color gradient indicates a generally older stellar population, with a slightly redder hue dominating the composition. There may be some minor asymmetry present, though the high smoothness fraction indicates this asymmetry is not due to any major mergers.
