The galaxy presents as a relatively smooth, centrally concentrated object with a roughly elliptical morphology. A dominant, yellowish central bulge is apparent, gradually fading into a less defined outer region with hints of greenish coloration. No distinct spiral arm structures or prominent dust lanes are discernible within the observable features. There is no evidence of major morphological disturbance or ongoing merger activity. The general appearance suggests a galaxy with a mature stellar population and relatively low levels of current star formation. The galaxy appears to have a large mass and the light is red-shifted.
