The galaxy presents a largely smooth morphology, appearing relatively featureless in the optical wavelengths captured in this image. It exhibits an approximately elliptical shape, showing an intermediate degree of ellipticity. There is a hint of some disturbance in the galaxy. The light is centrally concentrated, with intensity decreasing gradually towards the outer regions. The color profile suggests a population of older stars. The diameter is relatively small, with a radius of approximately 5 kpc. There is evidence of a merger event occurring.
