The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth, oval morphology. The light distribution shows a strong central concentration, with the brightness decreasing gradually outwards. The core region presents a yellowish-orange hue, suggesting an older stellar population. Fainter blue-ish halos extend from the core. There is no prominent disk structure visible and no signs of spiral arms or dust lanes are detected. There is no apparent ongoing merging activity or tidal disturbance. 
