The galaxy presents as a somewhat elliptical, centrally concentrated object with a smooth overall appearance. It exhibits a dominant, rounded morphology, showing minimal disc-like structure. There is faint evidence of a tidal tail or plume on the lower right side of the galaxy. The overall color profile suggests a population of older stars, with a redder hue concentrated toward the core. There is evidence of an ongoing or recent merger event, with significant morphological disturbance. The galaxy shows signs of merging, with the possibility of major disturbances. The light distribution appears relatively uniform, indicating a lack of significant internal structure or star formation regions.
