The galaxy appears to be an elliptical type, characterized by a smooth, centrally concentrated distribution of light. There is a lack of discernible spiral arm structure or dust lanes. The color profile indicates a population of older stars, evidenced by the yellowish-red hue, with a slight decrease in color and intensity as you move to the outer edges of the galaxy. The general shape is slightly oblate with no tidal tails or major distortions. The galaxy does not appear to be strongly interacting with any neighboring objects, but a deeper analysis of the surrounding field could reveal subtle disturbances.
