The galaxy presents a predominantly smooth, elliptical morphology. The light distribution appears centrally concentrated with a gradual decline in intensity towards the outer regions. While the overall shape approximates a circular form, subtle irregularities hint at possible minor disturbances within the galactic structure. The galaxy exhibits a reddish-yellow hue, suggesting an older stellar population and suppressed star formation. There may be some signs of a merger in its past due to the slight irregularities in its smooth structure. 
