The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated, bright central bulge that gradually diffuses outward. The color profile suggests a population of older stars, leaning toward redder wavelengths. There is no clear evidence of spiral arms or significant dust lanes. The overall structure appears undisturbed, lacking any obvious signs of ongoing mergers or tidal interactions. The galaxy shows a high degree of circularity. There is only a small suggestion of a disturbance or merger, without any distinct features.
