The galaxy presents as a relatively smooth, elliptical structure. Its shape is somewhat elongated, exhibiting a clear major and minor axis. The central region displays a concentrated, bright core that gradually diffuses outward. The overall color appears to be on the redder side, suggesting an older stellar population. While there's no immediately obvious spiral structure, there might be a subtle, faint disk component present, but is not clear in the image. Based on its smooth appearance and the lack of prominent star-forming regions, the galaxy is likely undergoing little to no active star formation. There appears to be no evidence of any major ongoing merger activity or significant morphological disturbance.
