The galaxy presents a largely smooth morphology. It appears as a rounded, concentrated central region with a faint, diffuse halo. There is a slight elongation, but it is close to being circular. Faint features, possibly minor tidal disturbances or spiral arm remnants, are suggested in the surrounding regions, with the main component being an undisturbed centralized, slightly elongated spheroid. Color gradients suggest a moderately old stellar population, concentrated towards the center with bluer components further out, which also indicate ongoing but relatively subdued star formation. The object is estimated to be a medium-mass system.
