The galaxy presents as a centrally concentrated object with a generally smooth morphology. The light profile appears relatively uniform, lacking prominent spiral arms or a distinct bar structure. The shape is mostly in between round and elliptical, displaying a slight elongation. There is a hint of a blueish tint. This suggests ongoing, though subdued, star formation. There is no obvious evidence of any major merging activity, or any major disturbances of any kind. The relative smoothness and concentration of light implies a possible early-type classification.
