The galaxy presents an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. A slight flattening is observed, suggesting it is not perfectly spherical. The core region displays a bright, yellowish hue, possibly indicative of an older stellar population. Fainter, diffuse blue emission is present in the outer regions which would imply some level of recent star formation. There is no evidence of strong tidal features or major disturbances, although the presence of some minor disturbances cannot be ruled out. The overall color gradients suggest a relatively quiescent system, with star formation largely suppressed or occurring at a low rate.
