The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a high degree of central concentration of light. The galaxy presents as predominantly spheroidal with a bright, yellowish core, suggesting an older stellar population. There is minimal indication of significant star formation activity or prominent spiral arm structures. The isophotes are largely regular and concentric, indicating a relaxed, dynamically evolved system with minimal signs of recent merger activity or tidal disturbances. The galaxy displays an overall rounded morphology. The faintness of the outer regions of the galaxy may indicate low surface brightness features.
