The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. There is no discernible disk component or spiral arm structure. The light distribution suggests a relatively uniform stellar population, without prominent knots of star formation. The galaxy exhibits a slightly elongated shape. There is no obvious indication of tidal features or ongoing merger activity, although a minor disturbance cannot be ruled out at this resolution. The overall color is consistent with an older stellar population, and there is no presence of dust obscuration or regions of intense star formation.
