The galaxy presents as a concentrated, ellipsoidal structure with a smooth light distribution. The central region exhibits a high degree of luminosity, gradually diminishing outwards. There appears to be little to no indication of spiral arm structures or significant disk features. The object displays a generally round morphology with no evidence of major disturbances or ongoing mergers. The color is predominantly red-shifted, suggesting an older stellar population and reduced ongoing star formation. There are no prominent dust lanes or regions of intense blue star formation visible in the image. Overall, the galaxy appears to be a relatively quiescent, evolved system.
