The galaxy presents as a smooth, centrally concentrated object, likely an elliptical. The core exhibits a yellowish hue, suggesting an older stellar population.  Surrounding the core is a more diffuse, bluish halo.  The galaxy is not perfectly spherical, displaying a slightly elongated, oval shape. There is no evidence of spiral arms or significant dust lanes. No obvious tidal features or distortions are apparent, suggesting a dynamically relaxed system, without any indication of a recent major merger or strong gravitational interaction. The galaxy appears relatively isolated, exhibiting no close companions within the immediate field of view.  The smooth morphology is consistent with a galaxy dominated by random stellar motions.
