The galaxy presents as a generally smooth, elliptical-like structure. The light is concentrated towards the center, suggesting a dense nucleus. The central region exhibits a yellowish-white hue, which might be indicative of an older stellar population. There is a very faint, bluish extension on one side, perhaps indicating a slight disk-like structure. The main body of the galaxy appears moderately elliptical rather than perfectly spherical, trending toward a somewhat flattened shape. Overall, the galaxy seems relatively undisturbed, lacking strong evidence of recent major merger events.
