The galaxy appears as a centrally concentrated object, largely smooth in texture with minimal discernible structure. The light distribution suggests a near-spherical morphology. Coloration is primarily yellowish-white, with a slightly redder core potentially indicative of an older stellar population. There is no evidence of spiral arms or a distinct galactic disk. There are no signs of any ongoing major merger events or significant tidal disturbances. The galaxy does not appear to be highly active in terms of star formation. The object's shape is generally round. There is no obvious elongation.
