The galaxy appears as a centrally concentrated object with a smooth, diffuse morphology, characteristic of an elliptical galaxy. The core exhibits a bright, yellowish hue, suggesting an older stellar population. There is some evidence of a surrounding halo or envelope, though it appears faint and without discernible substructure. The outer regions exhibit a slightly redder tone compared to the core, possibly indicating the presence of a population of older, cooler stars. No spiral arms or distinct disk features are visible in the image, suggesting a generally spheroidal structure. There is no obvious evidence of ongoing major merger activity or strong tidal interactions. The general impression is that of a relatively evolved, quiescent galaxy.
