The galaxy presents as a relatively smooth and centrally concentrated object, characterized by an elliptical morphology. The light distribution appears consistent with a de Vaucouleurs profile, suggesting an older stellar population dominating the light output. The color profile appears generally uniform across the galaxy, showing little evidence of significant dust lanes or prominent star-forming regions. The galaxy exhibits a high degree of circularity, indicating minimal signs of recent merger activity or tidal disturbances. There is no apparent spiral structure or bar feature within the galaxy's morphology.