The galaxy presents as a roughly elliptical form with a smooth, relatively featureless appearance. There are subtle color variations indicating some non-uniformity in stellar populations or dust distribution, however no distinct spiral arms or bar structures are discernible in the available image. The light is concentrated towards the center of the galaxy and the overall roundness of the light suggests it is most likely an elliptical galaxy. There does not appear to be evidence of significant tidal distortions or ongoing major mergers, although a slight asymmetry could indicate minor gravitational interactions or past accretion events.
