The galaxy presents as a somewhat faint and compact object. It exhibits a flattened, elliptical morphology. The light distribution within the galaxy appears relatively smooth and centrally concentrated, indicative of an older stellar population with little active star formation. There is a hint of subtle disturbances in the morphology, which might suggest a possible minor merger event in its past. The galaxy appears to be slightly elongated. The galaxy appears to lack prominent spiral arms or other defined structures and is primarily a collection of aging stars.
