The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is elliptical, appearing somewhere between round and slightly elongated, showing a subtle departure from perfect circularity. The light distribution suggests a fairly uniform structure, with the brightest region concentrated towards the galaxy's core. The core itself appears as a compact, bright region. The colours are mostly homogenous with a slight shift from green to red closer to the core, suggesting the possibility of older stellar populations dominating the nuclear region. The outer regions appear to fade gradually into the background. There's little evidence of significant star formation regions, strong dust lanes, or tidal disturbances, indicating a lack of recent major merging events.
