The galaxy appears to be a relatively compact elliptical galaxy. It presents a smooth, centrally concentrated morphology with a bright core that fades gradually outwards. There's no discernible disk component or spiral arm structure visible. The overall color index suggests a population dominated by older stars, giving it a slightly reddish hue, with indications of some ongoing star formation. Its shape is close to round with minimal asymmetry or tidal disturbances. The galaxy's structure suggests it is not currently undergoing a major merging event, but there may be some minor interactions or disturbances affecting its outer regions.
