The galaxy presents as a relatively smooth, centrally concentrated structure, appearing elliptical in shape. The central region exhibits a bright, yellowish-orange hue, suggesting an older stellar population. The galaxy's luminosity gradually decreases towards its outer edges, which appear less defined. There is very little evidence of spiral arm structures or significant dust lanes within the visible portion of the galaxy. The overall impression is that of a mature system, likely an elliptical galaxy with limited ongoing star formation.
