The galaxy presents as a relatively smooth, elliptical-like structure, with a concentrated central bulge exhibiting a yellow-white hue, indicative of an older stellar population. The light appears less blue than other galaxies, which may point to less active star formation. There is a minor redder clump that may indicate low-level star formation in a small region of the galaxy. The galaxy demonstrates a generally round appearance, with a slight deviation towards an oblong shape. There is no apparent sign of any major tidal disturbances or mergers, however the color gradients suggest that the material is not entirely homogenous. The overall morphology is indicative of a galaxy that has largely completed its primary star formation phase and is evolving towards a more quiescent state.
