The galaxy appears to be a relatively smooth, elongated system. Its morphology is suggestive of a highly elongated elliptical galaxy. The central region exhibits a concentrated, bright core, with a yellow-red hue indicative of an older stellar population or significant dust obscuration. The outer regions fade gradually, displaying a subtle blue tinge that suggests a possible presence of younger stars in the outer edges, or a lack of dust. There is no obvious evidence of spiral arm structure or significant star formation regions. No major disturbances or tidal features are readily apparent, suggesting it is not undergoing a major merger or significant interaction with another galaxy. 
