The galaxy presents a largely smooth morphology, suggestive of an elliptical galaxy. There appears to be no prominent disk structure or spiral arms. The shape is generally ellipsoidal, appearing more elongated than perfectly circular. There is no evidence of significant tidal disturbances or ongoing major mergers. The central region is bright and concentrated, decreasing in luminosity towards the outer edges. The color profile indicates a redder hue, which is consistent with an older stellar population, suggesting that star formation is currently low. 
