The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a roughly elliptical morphology, appearing more rounded than elongated. There is a suggestion of a slightly brighter core region, though it is not sharply defined. The color profile indicates a bias toward redder hues, which could be indicative of an older stellar population and/or a significant dust component within the galaxy. There is no immediately visible evidence of significant spiral arm structure or ongoing major merger activity based on the smooth overall appearance, though minor disturbances cannot be ruled out.
