The galaxy presents as a largely featureless, elliptical-like structure. Its light profile appears smooth and concentrated towards the center, suggesting an older stellar population. The dominant color is a yellowish hue, indicative of evolved stars. There is minimal evidence of spiral arms or dust lanes. The galaxy exhibits a high degree of roundness, lacking any pronounced elongation. No significant signs of tidal disturbances or ongoing merger activity are discernible. Its overall morphology suggests a relatively quiescent galaxy with a suppressed star formation rate.
