The galaxy presents as a single, concentrated object, likely an elliptical galaxy given its generally smooth and rounded appearance. The light distribution appears centrally concentrated, diminishing gradually towards the outer edges. The galaxy's color index suggests a relatively older stellar population, indicated by the slightly redder hue; this further supports its classification as an elliptical galaxy. There is no apparent spiral structure, bar, or dust lane features visible, reinforcing its smooth morphology. The overall luminosity indicates it is a relatively massive galaxy with ongoing, albeit potentially low-level, star formation. There is no visual evidence of any major mergers or significant tidal disturbances. The galaxy's general morphology is consistent with a relaxed system nearing the final stages of its evolution.
