The galaxy presents as a centrally concentrated, largely featureless object. It exhibits a generally smooth morphology, with a high degree of circularity. There is a slight elongation and a hint of a faint, diffuse halo extending beyond the main body. The color profile suggests a relatively evolved stellar population, with a yellowish-red hue dominating the central region. No spiral arms or dust lanes are discernible. There is no evidence of major ongoing mergers or significant tidal disturbances. The object has a relatively high degree of central concentration.
