The galaxy presents as a relatively smooth, centrally concentrated object. Its shape is generally round, with minimal distortion or elongation. There is a dominant central bulge region that emits strongly across the observed wavelengths, indicating a high density of stars. Some faint features possibly indicative of spiral arms or tidal disturbances are present, but the dominant characteristic is its smooth morphology. Overall, the galaxy appears to be a massive system with a modest ongoing star formation rate and a significant stellar mass. Some small fraction of the galaxy might be undergoing a merger event.
