The galaxy appears to be a relatively compact object. It exhibits a generally smooth morphology, with no readily discernible spiral arms or bar structure. The shape is largely round. Faint disturbances or irregularities appear to be present in the galaxy's morphology, and may suggest a possible interaction or merger. The galaxy's color index suggests a relatively evolved stellar population. However, the presence of some bluer regions indicates the presence of younger stars, and star formation. There is a faint halo around the galaxy.
