The galaxy presents as a centrally concentrated object. It appears smooth and elliptical in shape with a lack of distinct spiral arm structures. The color profile suggests a population of older stars, with a yellowish hue dominating. There is no evidence of active star formation regions or significant dust lanes. The galaxy displays a high degree of central concentration, indicating a dynamically relaxed system. There are no signs of tidal disturbances or ongoing mergers. The galaxy exhibits a seemingly uniform morphology, lacking features such as bars or rings.
