The galaxy exhibits an elliptical morphology, appearing somewhat flattened along its major axis. A bright, concentrated nucleus dominates the central region. The galaxy's light profile indicates a relatively smooth distribution, lacking prominent spiral arms or distinct structural features. There is a slight hint of possible minor disturbances in the outer regions. The colors suggest a population of older stars, with a relatively weak contribution from younger, bluer stars. Evidence of an ongoing or recent merger event is somewhat apparent, showing a hint of disturbance. The object is compact with a fairly small radius.
