The galaxy presents a predominantly smooth and featureless morphology, characteristic of an elliptical or S0-type galaxy. The light distribution is concentrated towards the center, forming a bright nucleus that transitions into a more diffuse halo. The overall shape appears somewhat flattened, deviating slightly from a perfect sphere. There are hints of a subtle disk-like structure, although this is not well-defined. Color gradients suggest a redder population of stars is dominant, with a possible contribution of bluer stars in the outer regions. There is no evidence of ongoing major merging activity or significant tidal disturbances. The image suggests this is a relatively evolved galaxy with low levels of active star formation.
