The galaxy appears as a centrally concentrated, smooth object, consistent with an elliptical morphology. There is no apparent spiral arm structure or dust lane obscuration visible. The overall color profile suggests a redder population of stars, concentrated towards the center. The lack of prominent blue regions implies relatively low on-going star formation. The galaxy has a generally round appearance, lacking any significant elongation or bar-like structure. There are no obvious signs of recent major mergers or tidal disturbances.
