The galaxy appears as a centrally concentrated object, exhibiting a relatively smooth morphology. Its core region displays a yellowish-orange hue, indicative of an older stellar population, potentially dominated by red giant stars. There is no clear spiral arm structure visible, and the overall shape is elliptical, trending toward a circular appearance. Evidence suggests a major merger, given the shape. While appearing smooth overall, the even light distribution is not fully uniform, likely due to disturbances from the aforementioned merger. The galaxy's light profile fades gradually from the core outward, suggesting a lack of active star formation in the outer regions. Based on the light emitted, there are potentially massive stars or supermassive black holes contained within.
