The galaxy appears to be a relatively compact system, exhibiting a largely smooth morphology. It has a roughly circular shape, with a gradual falloff in surface brightness from the center outwards. The galaxy's light distribution appears relatively uniform, suggesting it is an elliptical galaxy. There are no prominent spiral arms or bar structures visible. Faint irregularities in the outer regions are suggestive of minor disturbances, possibly resulting from past or ongoing interactions with smaller galaxies. No clear signs of a major merger are apparent. The galaxy appears to be a redder color, indicating an older stellar population. 
