The galaxy presents a largely smooth and elliptical morphology. Its light is concentrated towards the center, suggesting a prominent bulge. There is little evidence of spiral arm structure, but the color of the light suggests the presence of a population of older stars, typical of an elliptical galaxy. The galaxy's profile indicates it is generally round. There is no obvious sign of major disturbances or ongoing mergers. The overall appearance suggests a galaxy that is relatively quiescent in terms of recent star formation.
