The galaxy presents as a relatively smooth, elliptical structure. There is a centrally concentrated bulge, which appears yellowish-white, indicating a population of older stars. Moving outwards from the center, the galaxy appears bluer, possibly due to the presence of a younger stellar population and some ongoing star formation. The overall shape is somewhat elongated, but not excessively so. There is no obvious indication of a spiral arm structure or any major ongoing merger events, though a minor interaction or disturbance cannot be ruled out based on the image alone.
