The galaxy presents as a centrally concentrated object, exhibiting a smooth, relatively featureless morphology. The light profile appears to be consistent with a bulge-dominated system. The galaxy displays a roughly elliptical shape, appearing moderately rounded, rather than highly flattened or elongated. There is little evidence of spiral arm structures or strong tidal disturbances. The color gradient suggests a generally older stellar population, with the central bulge potentially composed of even older, redder stars and potentially a supermassive black hole at its center. The system lacks any apparent active star formation or prominent dust lanes. Overall, this galaxy is likely a massive, evolved system that has largely exhausted its gas supply.
