The galaxy presents as a single, relatively smooth, centrally concentrated object. The color appears to be a somewhat uniform yellow-orange hue. This suggests a lack of significant ongoing star formation and a relatively older stellar population. The apparent lack of spiral arms or a distinct disk structure further supports this classification. There is a slight elongation which could suggest a mild disturbance. There appears to be a smaller, secondary object close to the galaxy. While it could potentially be a foreground star, the proximity to the central galaxy leaves open the possibility of the object being a satellite galaxy. Further investigation is required to verify.
